 |
1 |
Abel, T., Bryan, G.L.,
and Norman, M.L., “The Formation and Fragmentation of Primordial
Molecular Clouds”, Astrophys. J.,
540, 39-44, (2000). Related online
version (cited on 7 February 2000):
 http://arXiv.org/abs/astro-ph/0002135.
|
|
2 |
Abel, T., Bryan, G.L.,
and Norman, M.L., “The formation of the first star in the
universe”, Science, 295, 93-98, (2002). Related online version (cited
on 4 December 2001):
http://arXiv.org/abs/astro-ph/0112088.
|
|
3 |
Akiyama, S., and
Wheeler, J.C., “Magnetic Fields in Supernovae”, in Fryer, C.L.,
ed., Stellar Collapse, Proceedings of “Core Collapse of Massive
Stars”, 200th AAS meeting, Albuquerque, NM, June 2002, vol. 302 of
Astrophysics and Space Science Library, (Kluwer Academic
Publishers, Dordrecht, Netherlands; Boston, U.S.A., 2004). Related
online version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0211458.
|
|
4 |
Alcubierre,
M., Brügmann, B., Holz, D.E., Takahashi, R., Brandt, S., Seidel,
E., and Thornburg, J., “Symmetry without symmetry: Numerical
simulation of axisymmetric systems using Cartesian grids”,
Int. J. Mod. Phys. D, 10, 273-289, (2001). Related online version (cited
on 4 August 1999):
http://arXiv.org/abs/gr-qc/9908012.
|
|
5 |
Andersson,
N., “A new class of unstable modes of rotating relativistic stars”,
Astrophys. J., 502, 708-713, (1998). Related online version
(cited on 24 June 1997):
http://arXiv.org/abs/gr-qc/9706075.
|
|
6 |
Andersson, N.,
“Gravitational waves from instabilities in relativistic stars”,
Class. Quantum Grav., 20, R105-R144,
(2002). URL (cited on 4 November 2002):
http://arXiv.org/abs/astro-ph/0211057.
|
|
7 |
Arnaud, N., Barsuglia, M.,
Bizouard, M.-A., Brisson, V., Cavalier, F., Davier, M., Hello, P.,
Kreckelbergh, S., and Porter, E., “Detection of a close supernova
gravitational wave burst in a network of interferometers, neutrino
and optical detectors”, Astropart.
Phys., 21, 201-221, (2004).
|
|
8 |
Arnett, W.D.,
Bahcall, J. N., Kirshner, R.P., and Woosley, S.E., “Supernova
1987a”, Annu. Rev. Astron. Astrophys., 27, 629-700, (1989).
|
|
9 |
Arras, P., Flanagan,
É.É., Morsink, S.M., Schenk, A.K., Teukolsky, S.A., and Wasserman,
I., “Saturation of the r-mode
instability”, Astrophys. J.,
591, 1129-1151, (2002). Related online
version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0202345.
|
|
10 |
Baraffe, I.,
Heger, A., and Woosley, S.E., “On the stability of very massive
supermassive stars”, Astrophys. J.,
550, 890-896, (2001). Related online
version (cited on 26 September 2000):
http://arXiv.org/abs/astro-ph/0009410.
|
|
11 |
Bardeen, M., and
Piran, T., “General relativistic axisymmetric rotating systems:
Coordinates and equations”, Phys.
Rep., 96, 205-250, (1983).
|
|
12 |
Baron, E.,
Cooperstein, J., and Kahana, S., “Supernovae and the nuclear
equation of state at high densities”, Nucl.
Phys. A, 440, 744-754, (1985).
|
|
13 |
Baron, E.,
Cooperstein, J., and Kahana, S., “Type II supernovae in
12M and 15M
stars: The equation of state and general relativity”, Phys. Rev. Lett., 55,
126-129, (1985).
|
|
14 |
Baron, E.,
Cooperstein, J., Kahana, S., and Nomoto, K., “Collapsing white
dwarfs”, Astrophys. J., 320, 304-307,
(1987).
|
|
15 |
Baumgarte, T.W., Janka, H.-T., Keil, W., Shapiro,
S.L., and Teukolsky, S.A., “Delayed Collapse of Hot Neutron Stars
to Black Holes via Hadronic Phase Transitions”, Astrophys. J., 468,
823-833, (1996).
|
|
16 |
Baumgarte,
T.W., and Shapiro, S.L., “Evolution of rotating supermassive stars
to the onset of collapse”, Astrophys.
J., 526, 941-952, (1999).
Related online version (cited on 14 September 1999):
http://arXiv.org/abs/astro-ph/9909237.
|
|
17 |
Baumgarte,
T.W., and Shapiro, S.L., “Collapse of a Magnetized Star to a Black
Hole”, Astrophys. J., 585, 930-947, (2003). URL (cited on 14 November
2002):
http://arXiv.org/abs/astro-ph/0211339.
|
|
18 |
Baumgarte,
T.W., Shapiro, S.L., and Teukolsky, S.A., “Computing supernova
collapse to neutron stars and black holes”, Astrophys. J., 443,
717-734, (1995).
|
|
19 |
Baumgarte,
T.W., Shapiro, S.L., and Teukolsky, S.A., “Computing the Delayed
Collapse of Hot Neutron Stars to Black Holes”, Astrophys. J., 458,
680-691, (1996).
|
|
20 |
Bazan, G., and Arnett,
D., “Convection, nucleosynthesis, and core collapse”, Astrophys. J. Lett.,
433, L41-L43, (1994).
|
|
21 |
Begelman, M.C.,
and Rees, M.J., “The fate of dense stellar systems”, Mon. Not. R. Astron. Soc., 185, 847-860,
(1978).
|
|
22 |
Berger, E.,
Kulkarni, S.R., Frail, D.A., and Soderberg, A.M., “A Radio Survey
of Type Ib and Ic Supernovae: Searching for Engine-driven
Supernovae”, Astrophys. J.,
599, 408-418, (2003).
|
|
23 |
Bethe, H.A., “Supernova
mechanisms”, Rev. Mod. Phys.,
62, 801-866, (1990).
|
|
24 |
Bethe, H.A., and
Wilson, J.R., “Revival of a stalled supernova shock by neutrino
heating”, Astrophys. J., 295, 14-23, (1985).
|
|
25 |
Blanchet, L.,
Damour, T., and Schäfer, G., “Post-Newtonian hydrodynamics and
post-Newtonian gravitational wave generation for numerical
relativity”, Mon. Not. R. Astron.
Soc., 242, 289-305, (1990).
|
|
26 |
Blondin, J.M.,
Mezzacappa, A., and DeMarino, C., “Stability of Standing Accretion
Shocks, with an Eye toward Core-Collapse Supernovae”, Astrophys. J., 584,
971-980, (2003).
|
|
27 |
Bodenheimer, P., and Ostriker, J.P., “Rapidly
rotating stars. VIII. Zero-viscosity polytropic sequences”,
Astrophys. J., 180, 159-170, (1973).
|
|
28 |
Bonazzola, S.,
and Marck, J.-A., “Efficiency of gravitational radiation from
axisymmetric and 3D stellar collapse. I - Polytropic case”,
Astron. Astrophys., 267, 623-633, (1993).
|
|
29 |
Bowers, R.L.,
and Wilson, J.R., “Collapse of iron stellar cores”, Astrophys. J., 263,
366-376, (1982).
|
|
30 |
Bowers, R.L., and
Wilson, J.R., “A numerical model for stellar core collapse”,
Astrophys. J. Suppl. Ser., 50,
115-159, (1982).
|
|
31 |
Brachwitz,
F., Dean, D.J., Hix, W.R., Iwamoto, K., Langanke, K.,
Martínez-Pinedo, G., Nomoto, K., Strayer, M.R., Thielemann, F.-K.,
and Umeda, H., “The role of electron captures in Chandrasekhar-mass
models for Type Ia supernovae”, Astrophys.
J., 536, 934-947, (2000).
Related online version (cited on 26 January 2000):
http://arXiv.org/abs/astro-ph/0001464.
|
|
32 |
Bravo, E., and
García-Senz, D., “Coulomb corrections to the equation of state of
nuclear statistical equilibrium matter: Implications for SNIa
nucleosynthesis and the accretion-induced collapse of white
dwarfs”, Mon. Not. R. Astron. Soc.,
307, 984-992, (1999).
|
|
33 |
Bromm, V., Coppi, P.S.,
and Larson, R.B., “Forming the first stars in the universe: The
fragmentation of primordial gas”, Astrophys.
J. Lett., 527, L5-L8, (1999).
Related online version (cited on 13 October 1999):
http://arXiv.org/abs/astro-ph/9910224.
|
|
34 |
Brown, J.D.,
“Gravitational waves from the dynamical bar instability in a
rapidly rotating star”, Phys. Rev. D,
62, 084024-1-11, (2000). Related
online version (cited on 1 April 2000):
http://arXiv.org/abs/gr-qc/0004002.
|
|
35 |
Brown, J.D.,
“Rotational instabilities in post-collapse stellar cores”, in
Centrella, J.M., ed., Astrophysical Sources
for Ground-Based Gravitational Wave Detectors, Philadelphia,
Pennsylvania, 30 October - 1 November 2000, AIP Conference
Proceedings, 234-245, (American Institute of Physics, Melville,
U.S.A., 2001).
|
|
36 |
Bruenn, S.W.,
“Numerical simulations of core collapse supernovae”, in Guidry,
M.W., and Strayer, M.R., eds., Nuclear
Physics in the Universe, Proceedings of the First Symposium
on Nuclear Physics in the Universe held in Oak Ridge, Tennessee,
USA, 24-26 September 1992, 31-50, (Institute of Physics, Bristol,
U.K.; Philadelphia, U.S.A., 1993).
|
|
37 |
Bruenn, S.W.,
De Nisco, K.R., and Mezzacappa, A., “General relativistic
effects in the core collapse supernova mechanism”, Astrophys. J., 560,
326-338, (2001). Related online version (cited on 23 January
2001):
http://arXiv.org/abs/astro-ph/0101400.
|
|
38 |
Buonanno, A.,
Sigl, G., Raffelt, G.G., Janka, H.-T., and Müller, E., “Stochastic
gravitational-wave background from cosmological supernovae”,
Phys. Rev. D, 72, 084001, (2005).
|
|
39 |
Buras, R., Rampp, M.,
Janka, H.-T., and Kifonidis, K., “Improved Models of Stellar Core
Collapse and Still No Explosions: What Is Missing?”, Phys. Rev. Lett., 90,
241101-1-4, (2003).
|
|
40 |
Burrows, A.,
personal communication, (2005).
|
|
41 |
Burrows, A., and
Hayes, J., “Pulsar recoil and gravitational radiation due to
asymmetrical stellar collapse and explosion”, Phys. Rev. Lett., 76,
352-355, (1996).
|
|
42 |
Burrows, A.,
Hayes, J., and Fryxell, B.A., “On the Nature of Core-Collapse
Supernova Explosions”, Astrophys. J.,
450, 830-850, (1995).
|
|
43 |
Burrows, A., Livne,
E., Dessart, L., Ott, C., and Murphy, J., “A New Mechanism for
Core-Collapse Supernova Explosions”, Astrophys. J., accepted, (2005). Related online
version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0510687.
|
|
44 |
Burrows, A., and
Thompson, T.A., “Neutrino-Matter Interaction Rates in Supernovae”,
in Fryer, C.L., ed., Stellar Collapse,
Proceedings of “Core Collapse of Massive Stars”, 200th AAS meeting,
Albuquerque, NM, June 2002, vol. 302 of Astrophysics and Space
Science Library, (Kluwer Academic Publishers, Dordrecht,
Netherlands; Boston, U.S.A., 2004). Related online version (cited
on 21 December 2005):
http://arXiv.org/abs/astro-ph/0211404.
|
|
45 |
California Institute of
Technology, “LIGO Laboratory Home Page”, project homepage. URL
(cited on 4 October 2002):
http://www.ligo.caltech.edu.
|
|
46 |
Cappellaro,
E., Evans, R., and Turatto, M., “A new determination of supernova
rates and a comparison with indicators for galactic star
formation”, Astron. Astrophys.,
351, 459-466, (1999).
|
|
47 |
Carr, B.J., Bond,
J.R., and Arnett, W.D., “Cosmological consequences of population
III stars”, Astrophys. J.,
277, 445-469, (1984).
|
|
48 |
Cassisi, S.,
Iben Jr, I., and Tornambé, A., “Hydrogen-accreting
carbon-oxygen white dwarfs”, Astrophys.
J., 496, 376-385, (1998).
|
|
49 |
Centrella,
J.M., New, K.C.B., Lowe, L., and Brown, J.D., “Dynamical rotational
instability at low T/W”, Astrophys. J. Lett., 550, L193-L196, (2001). Related online version
(cited on 27 October 2000):
http://arXiv.org/abs/astro-ph/0010574.
|
|
50 |
Chandrasekhar, S., “Dynamical Instability of
Gaseous Masses Approaching the Schwarzschild Limit in General
Relativity”, Phys. Rev. Lett.,
12, 114-116, (1964). Erratum 437-438.
|
|
51 |
Chandrasekhar, S., “The dynamical
instability of gaseous masses approaching the Schwarzschild limit
in general relativity”, Astrophys. J.,
140, 417-433, (1964).
|
|
52 |
Chandrasekhar, S.,
An Introduction to the Study of Stellar
Structure, (Dover, New York, U.S.A., 1967).
|
|
53 |
Colgate, S.A.,
“Supernova: Hot bubbles drive explosions”, Nature, 341, 489-490,
(1989).
|
|
54 |
Colgate, S.A.,
Herant, M., and Benz, W., “Neutron star accretion and the neutrino
fireball”, Phys. Rep., 227, 157-174, (1993).
|
|
55 |
Colgate, S.A.,
and White, R.H., “The hydrodynamic behavior of supernovae
explosions”, Astrophys. J.,
143, 626-681, (1966).
|
|
56 |
Cook, G.B., Shapiro,
S.L., and Teukolsky, S.A., “Testing a simplified version of
Einstein’s equations for numerical relativity”, Phys. Rev. D, 53,
5533-5540, (1996). Related online version (cited on 5 December
1995):
http://arXiv.org/abs/astro-ph/9512009.
|
|
57 |
Detweiler, S.,
and Lindblom, L., “On the evolution of the homogeneous ellipsoidal
figures. II. Gravitational collapse and gravitational radiation”,
Astrophys. J., 250, 739-749, (1981).
|
|
58 |
Dimmelmeier, H., Font, J.A., and Müller, E.,
“Gravitational waves from relativistic rotational core collapse”,
Astrophys. J. Lett., 560, L163-L166, (2001). Related online version
(cited on 21 April 2001):
http://arXiv.org/abs/astro-ph/0103088.
|
|
59 |
Dimmelmeier, H., Font, J.A., and Müller, E.,
“Relativistic simulations of rotational core collapse. I. Methods,
initial models, and code tests”, Astron.
Astrophys., 388, 917-935,
(2002). Related online version (cited on 17 April 2002):
http://arXiv.org/abs/astro-ph/0204288.
|
|
60 |
Dimmelmeier, H., Font, J.A., and Müller, E.,
“Relativistic simulations of rotational core collapse. II. Collapse
dynamics and gravitational radiation”, Astron. Astrophys., 393, 523-542, (2002). Related online version
(cited on 17 April 2002):
http://arXiv.org/abs/astro-ph/0204289.
|
|
61 |
Dimmelmeier, H., Novak, J., Font, J.A., Ibáñez,
J.M., and Müller, E., “Combining spectral and shock-capturing
methods: A new numerical approach for 3D relativistic core collapse
simulations”, Astron. Astrophys.,
560, 163-166, (2005).
|
|
62 |
Duez, M.D., Shapiro,
S.L., and You, H.-J., “Relativistic hydrodynamic evolutions with
black hole excision”, Phys. Rev. D,
69, 104016, (2004).
|
|
63 |
Durisen, R.H.,
and Tohline, J.E., “Fission of rapidly rotating fluid systems”, in
Black, D., and Matthews, M., eds., Protostars
and Planets II, 534-575, (University of Arizona Press,
Tucson, U.S.A., 1985).
|
|
64 |
Eisenstein,
D.J., and Loeb, A., “Origin of quasar progenitors from the collapse
of low-spin cosmological perturbations”, Astrophys. J., 443,
11-17, (1995). Related online version (cited on 11 January
1994):
http://arXiv.org/abs/astro-ph/9401016.
|
|
65 |
Epstein, R.,
The post-Newtonian theory of the generation
of gravitational radiation and its application to stellar collapse, Ph.D. Thesis,
(Stanford University, Stanford, U.S.A., 1976).
|
|
66 |
Epstein, R., and
Wagoner, R.V., “Post-Newtonian generation of gravitational waves”,
Astrophys. J., 197, 717-723, (1975).
|
|
67 |
Eriguchi, Y., and
Müller, E., “Equilibrium models of differentially rotating
polytropes and the collapse of rotating stellar cores”,
Astron. Astrophys., 147, 161-168, (1985).
|
|
68 |
Ferrarese, L.,
and Merritt, D., “A fundamental relation between supermassive black
holes and their host galaxies”, Astrophys. J.
Lett., 539, L9-L12, (2000).
Related online version (cited on 4 June 2000):
http://arXiv.org/abs/astro-ph/0006053.
|
|
69 |
Ferrari, V.,
Matarrese, S., and Schneider, R., “Gravitational wave background
from a cosmological population of core-collapse supernovae”,
Mon. Not. R. Astron. Soc.,
303, 247-257, (1999). Related online
version (cited on 15 October 1998):
http://arXiv.org/abs/astro-ph/9804259.
|
|
70 |
Ferrari, V.,
Miniutti, G., and Pons, J.A., “Gravitational waves from newly born,
hot neutron stars”, Mon. Not. R. Astron.
Soc., 342, 629-638, (2003).
Related online version (cited on 26 October 2002):
http://arXiv.org/abs/astro-ph/0210581.
|
|
71 |
Finn, L.S.,
“Supernovae, gravitational radiation, and the quadrupole formula”,
in Evans, C.R., Finn, L.S., and Hobill, D.W., eds., Frontiers in Numerical Relativity, International
workshop devoted to research in numerical relativity, held in
Urbana-Champaign in May 1988, 126-145, (Cambridge University Press,
Cambridge, U.K.; New York, U.S.A., 1989).
|
|
72 |
Finn, L.S.,
“Detectability of gravitational radiation from stellar-core
collapse”, in Buchler, J.R., Detweiler, S., and Ipser, J.R., eds.,
Nonlinear problems in relativity and
cosmology, 6th Florida Workshop in Nonlinear Astronomy, held
on October 2-4, 1990 in Gainesville, Florida, 156-172, (New York
Academy of Sciences, New York, U.S.A., 1991).
|
|
73 |
Finn, L.S., “Gravitional
Radiation Sources and Signatures”, in Dixon, L.J., ed.,
Gravity: From the Hubble Length to the Planck Length,
Proceedings of the 26th SLAC Summer Institute on Particle Physics
(SSI 98), Stanford, USA, 3-14 August 1998, vol. 538 of SLAC-R,
(SLAC, Springfield, U.S.A., 2001). URL (cited on 30 March
1999):
http://www.slac.stanford.edu/pubs/confproc/ssi98/ssi98-007.html.
also at: http://arXiv.org/abs/gr-qc/9903107.
|
|
74 |
Finn, L.S., and Evans,
C.R., “Determining gravitational radiation from Newtonian
self-gravitating systems”, Astrophys.
J., 351, 588-600, (1990).
|
|
75 |
Foglizzo, T.,
Scheck, L., and Janka, H.-T., “Neutrino-driven convection versus
advection in core collapse supernovae”, Astron. Astrophys., submitted, (2005). Related
online version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0507636.
|
|
76 |
Folkner, W.M.,
ed., Laser Interferometer Space Antenna:
Second International LISA Symposium on
the Detection and Observation of Gravitational Waves in Space,
Pasadena 1998, vol. 456 of AIP Conference Proceedings,
(Springer, New York, U.S.A., 1993).
|
|
77 |
Friedman, J.L.,
and Morsink, S.M., “Axial instability of rotating relativistic
stars”, Astrophys. J., 502, 714-720,
(1998). Related online version (cited on 23 June 1997):
http://arXiv.org/abs/gr-qc/9706073.
|
|
78 |
Fryer, C.L., “Mass
Limits For Black Hole Formation”, Astrophys.
J., 522, 413-418, (1999).
|
|
79 |
Fryer, C.L., “Stellar
Collapse”, Int. J. Mod. Phys. D,
12, 1795-1835, (2003).
|
|
80 |
Fryer, C.L.,
“Neutron Star Kicks from Asymmetric Collapse”, Astrophys. J., 601,
L175-L178, (2004).
|
|
81 |
Fryer, C.L., ed.,
Stellar Collapse, Proceedings of “Core
Collapse of Massive Stars”, 200th AAS meeting, Albuquerque, NM,
June 2002, vol. 302 of Astrophysics and Space Science Library,
(Kluwer Academic Publishers, Dordrecht, Netherlands; Boston,
U.S.A., 2004).
|
|
82 |
Fryer, C.L., Benz,
W., Herant, M., and Colgate, S.A., “What can the accretion-induced
collapse of white dwarfs really explain?”, Astrophys. J., 516,
892-899, (1999). Related online version (cited on 2 December
1998):
http://arXiv.org/abs/astro-ph/9812058.
|
|
83 |
Fryer, C.L., and Heger,
A., “Core-Collapse Simulations of Rotating Stars”, Astrophys. J., 541,
1033-1050, (2000). Related online version (cited on 30 July
1999):
http://arXiv.org/abs/astro-ph/9907433.
|
|
84 |
Fryer, C.L.,
and Heger, A., “Binary Merger Progenitors for Gamma-Ray Bursts and
Hypernovae”, Astrophys. J.,
623, 302-313, (2005).
|
|
85 |
Fryer, C.L.,
Heger, A., Langer, N., and Wellstein, S., “Stellar Collapse”,
Int. J. Mod. Phys. D, 12, 1795-1835, (2003).
|
|
86 |
Fryer, C.L., Holz,
D.E., and Hughes, S.A., “Gravitational wave emission from
core-collapse of massive stars”, Astrophys.
J., 565, 430-446, (2002).
Related online version (cited on 25 September 2001):
http://arXiv.org/abs/astro-ph/0106113.
|
|
87 |
Fryer, C.L., Holz, D.E.,
and Hughes, S.A., “Gravitational Waves from Stellar Collapse:
Correlations to Explosion Asymmetries”, Astrophys. J., 609,
288-300, (2004).
|
|
88 |
Fryer, C.L., Holz,
D.E., Hughes, S.A., and Warren, M.S., “Stellar Collapse and
Gravitational Waves”, in Fryer, C.L., ed., Stellar Collapse, Proceedings of “Core Collapse of
Massive Stars”, 200th AAS meeting, Albuquerque, NM, June 2002, vol.
302 of Astrophysics and Space Science Library, (Kluwer Academic
Publishers, Dordrecht, Netherlands; Boston, U.S.A., 2004). Related
online version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0211609.
|
|
89 |
Fryer, C.L.,
and Kalogera, V., “Theoretical black hole mass distributions”,
Astrophys. J., 554, 548-560, (2001).
|
|
90 |
Fryer,
C.L., and Kusenko, A., “Effects of neutrino-driven kicks on the
supernova explosion mechanism”, Astrophys.
J., submitted, (2005). Related online version (cited on 21
December 2005):
http://arXiv.org/abs/astro-ph/0512033.
|
|
91 |
Fryer, C.L., and
Warren, M.S., “Modeling Core-Collapse Supernovae in Three
Dimensions”, Astrophys. J. Lett.,
574, L65-L68, (2002). URL (cited on 3
June 2002):
http://arXiv.org/abs/astro-ph/0206017.
|
|
92 |
Fryer,
C.L., and Warren, M.S., “The Collapse of Rotating Massive Stars in
Three Dimensions”, Astrophys. J.,
601, 391-404, (2004).
|
|
93 |
Fryer,
C.L., and Woosley, S.E., “Helium Star/Black Hole Mergers: A New
Gamma-Ray Burst Model”, Astrophys. J.,
502, L9-L12, (1998).
|
|
94 |
Fryer, C.L.,
Woosley, S.E., and Hartmann, D., “Formation Rates of Black Hole
Accretion Disk Gamma-Ray Bursts”, Astrophys.
J., 526, 152-177, (1999).
|
|
95 |
Fryer, C.L., Woosley, S.E.,
and Hartmann, D.H., “Formation Rates of Black Hole Accretion Disk
Gamma-Ray Bursts”, Astrophys. J.,
526, 152-177, (1999).
|
|
96 |
Fryer, C.L.,
Woosley, S.E., and Heger, A., “Pair-instability supernovae, gravity
waves, and gamma-ray transients”, Astrophys.
J., 550, 372-382, (2001).
Related online version (cited on 13 July 2000):
http://arXiv.org/abs/astro-ph/0007176.
|
|
97 |
Gressman, P.,
Lin, L.-M., Suen, W.-M., Stergioulas, N., and Friedman, J.L.,
“Nonlinear r-modes in neutron stars:
Instability of an unstable mode”, Phys. Rev.
D, 66, 041303-1-5, (2002).
|
|
98 |
Hachisu, I., “A
versatile method for obtaining structures of rapidly rotating
stars”, Astrophys. J. Suppl. Ser., 61,
479-507, (1986).
|
|
99 |
Haehnelt,
M.G., “Low-frequency gravitational waves from supermassive black
holes”, Mon. Not. R. Astron. Soc., 269, 199-208, (1994).
|
|
100 |
Haehnelt, M.G.,
Natarajan, P., and Rees, M.J., “High-redshift galaxies, their
active nuclei and central black holes”, Mon.
Not. R. Astron. Soc., 300,
817-827, (1998). Related online version (cited on 18 December
1997):
http://arXiv.org/abs/astro-ph/9712259.
|
|
101 |
Haehnelt, M.G.,
and Rees, M.J., “The formation of nuclei in newly formed galaxies
and the evolution of the quasar population”, Mon. Not. R. Astron. Soc., 263, 168-178, (1993).
|
|
102 |
Haensel, P.,
Levenfish, K.P., and Yakovlev, D.G., “Bulk viscosity in superfluid
neutron star cores. III. Effects of  - hyperons”, Astron.
Astrophys., 381, 1080-1089,
(2002). Related online version (cited on 26 October
2001):
http://arXiv.org/abs/astro-ph/0110575.
|
|
103 |
Hamuy, M., “Observed
and physical properties of core-collapse supernovae”, Astrophys. J., 582,
905-914, (2003). URL (cited on 10 September 2002):
http://arXiv.org/abs/astro-ph/0209174.
|
|
104 |
Hannover University, “GEO
600 home page”, project homepage. URL (cited on 4 October
2002):
http://www.geo600.uni-hannover.de/.
|
|
105 |
Hayashi, A.,
Eriguchi, Y., and Hashimoto, M., “On the possibility of the
nonexplosive core contraction of massive stars: New evolutionary
paths from rotating white dwarfs to rotating neutron stars”,
Astrophys. J., 492, 286-297, (1998).
|
|
106 |
Hayashi, A.,
Eriguchi, Y., and Hashimoto, M., “On the possibility of the
nonexplosive core contraction of massive stars. II. General
relativistic analysis”, Astrophys. J.,
521, 376-381, (1999).
|
|
107 |
Heger, A.,
The presupernova evolution of rotating
massive stars, Ph.D. Thesis, (Technische Universität
München, Munich, Germany, 1998).
|
|
108 |
Heger, A., Fryer, C.L.,
Woosley, S.E., Langer, N., and Hartmann, D.H., “How Massive Single
Stars End Their Life”, Astrophys. J.,
591, 288-300, (2001).
|
|
109 |
Heger, A., Langer, N.,
and Woosley, S.E., “Presupernova evolution of rotating massive
stars. I. Numerical method and evolution of the internal stellar
structure”, Astrophys. J.,
528, 368-396, (2000). Related online
version (cited on 12 April 1999):
http://arXiv.org/abs/astro-ph/9904132.
|
|
110 |
Heger, A., Woosley,
S.E., and Spruit, H.C., “Presupernova Evolution of Differentially
Rotating Massive Stars Including Magnetic Fields”, Astrophys. J., 626,
350-363, (2005).
|
|
111 |
Herant, M., “Inside
the Supernova: A Powerful Convective Engine”, Phys. Rep., 256,
117-133, (1995).
|
|
112 |
Herant, M., Benz, W.,
Hiz, W.R., Fryer, C.L., and Colgate, S.A., “Inside the Supernova: A
Powerful Convective Engine”, Astrophys.
J., 435, 339-361, (1994).
|
|
113 |
Hillebrandt, W., “Stellar Collapse and
Supernova Explosions”, in Pacini, F., ed., High Energy Phenomena around
Collapsed Stars, Proceedings of the NATO Advanced Study
Institute, Cargèse, Corsica, France, September 2-13, 1985, vol. 195
of NATO Science Series, 73-104, (Reidel, Dordrecht, Netherlands;
Boston, U.S.A., 1987).
|
|
114 |
Hillebrandt, W., Nomoto, K., and Wolff, R.G.,
“Supernova explosions of massive stars - The mass range 8 to 10
solar masses”, Astron. Astrophys.,
133, 175-184, (1984).
|
|
115 |
Ho, W.C.G., and Lai, D.,
“r-Mode oscillations and spin-down of
young rotating magnetic neutron stars”, Astrophys. J., 543,
386-394, (2000). Related online version (cited on 15 December
1999):
http://arXiv.org/abs/astro-ph/9912296.
|
|
116 |
Höflich, P.,
Khokhlov, A., Wang, L., Wheeler, J.C., and Baade, D., “Aspherical
Supernovae Explosions”, in van der Hucht, K.A., Herrero, A.,
and Esteban, C., eds., A Massive Star
Odyssey, from Main Sequence to
Supernova, Lanzarote, Canary Islands, Spain, June 24-28,
2002, vol. 212 of IAU Symposia, (Astronomical Society of the
Pacific, San Francisco, U.S.A., 2003). Related online version
(cited on 12 July 2002):
http://arXiv.org/abs/astro-ph/0207272.
|
|
117 |
Hogan, C.J., “A model
of pregalactic evolution”, Mon. Not. R.
Astron. Soc., 188, 781-790,
(1979).
|
|
118 |
Houser, J.L., “The
effect of rotation on the gravitational radiation and dynamical
instability of stiff stellar cores”, Mon.
Not. R. Astron. Soc., 299,
1069-1086, (1998).
|
|
119 |
Hughes, S.A.,
“Untangling the merger history of massive black holes with LISA”,
Mon. Not. R.
Astron. Soc., 331, 805-816,
(2002). Related online version (cited on 30 August 2001):
http://arXiv.org/abs/astro-ph/0108483.
|
|
120 |
Hughes, S.A., Márka,
S., Bender, P.L., and Hogan, C.J., “New physics and astronomy with
the new gravitational-wave observatories”, in Graf, N., ed.,
Proceedings of Snowmass 2001, The
Future of Particle Physics, 30 June - 21 July 2001, Snowmass
Village, Colorado, vol. C010630, P402, (SLAC eConf, Stanford,
U.S.A., 2001). URL (cited on 15 October 2001):
http://www.slac.stanford.edu/econf/C010630/proceedings.shtml.
|
|
121 |
Hungerford, A., Fryer, C.L., and Rockefeller, G.,
“Gamma Rays from Single-Lobe Supernova Explosions”, Astrophys. J., 635,
487-501, (2005).
|
|
122 |
Hungerford,
A., Fryer, C.L., and Warren, M.S., “Gamma Rays from Asymmetric
Supernovae”, Astrophys. J.,
594, 390-403, (2005).
|
|
123 |
Iben, I., “Massive stars
in quasi-static equilibrium”, Astrophys.
J., 138, 1090-1096, (1963).
|
|
124 |
Imamura, J.N.,
and Durisen, R.H., “The Dominance of Dynamic Barlike Instabilities
in the Evolution of a Massive Stellar Core Collapse That
“Fizzles””, Astrophys. J.,
549, 1062-1075, (2001).
|
|
125 |
Imamura, J.N.,
Friedman, J.L., and Durisen, R.H., “Secular stability limits for
rotating polytropic stars”, Astrophys.
J., 294, 474-478, (1985).
|
|
126 |
INFN, “The Virgo Project”,
project homepage. URL (cited on 4 October 2002):
http://www.virgo.infn.it/.
|
|
127 |
Isern, J., Canal, R.,
and Labay, J., “The outcome of explosive ignition of ONeMg cores:
supernovae, neutron stars, or “iron” white dwarfs?”, Astrophys. J. Lett., 372, L83-L86, (1991).
|
|
128 |
Janka, H.-T.,
“Conditions for shock revival by neutrino heating in core-collapse
supernovae”, Astron. Astrophys.,
368, 527-560, (2001). Related online
version (cited on 28 August 2000):
http://arXiv.org/abs/astro-ph/0008432.
|
|
129 |
Janka, H.-T.,
“Supermassive Stars: Fact or Fiction?”, in Chui, C.K., Siuniaev,
R.A., and Churazov, E., eds., Lighthouses of
the Universe: The Most Luminous Celestial Objects
and Their Use for Cosmology,
Proceedings of the MPA/ESO/MPE/USM Joint Astronomy Conference, held
in Garching, Germany, 6-10 August 2001, ESO Astrophysics Symposia,
357-368, (Springer, Berlin, Germany; New York, U.S.A., 2002).
Related online version (cited on 1 February 2002):
http://arXiv.org/abs/astro-ph/0202028.
|
|
130 |
Janka, H.-T., Buras,
R., Kifonidis, K., Rampp, M., and Plewa, T., “Explosion Mechanisms
of Massive Stars”, in Fryer, C.L., ed., Stellar Collapse, Proceedings of “Core Collapse of
Massive Stars”, 200th AAS meeting, Albuquerque, NM, June 2002, vol.
302 of Astrophysics and Space Science Library, (Kluwer Academic
Publishers, Dordrecht, Netherlands; Boston, U.S.A., 2004). Related
online version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0212314.
|
|
131 |
Janka, H.-T., and
Müller, E., “Neutrino-driven type-II supernovae: Neutrino heating
and post bounce dynamics”, in Suzuki, Y., and Nakamura, K., eds.,
Frontiers of Neutrino Astrophysics,
Proceedings of the International Symposium on Neutrino Astrophysics
held on October 19-22, 1992, Takayama / Kamioka, Japan, vol. 5
of Frontiers Science Series, 203-217, (Universal Academy Press,
Tokyo, Japan, 1993).
|
|
132 |
Janka, H.-T., and
Müller, E., “Dynamics of Type-II supernovae”, in McCray, R., and
Wang, Z., eds., Supernovae and Supernovae
Remnants, Proceedings of the IAU Colloquium 145, held in
Xian, China, May 24-29, 1993, 109-118, (Cambridge University Press,
Cambridge, U.K., 1996).
|
|
133 |
Janka, H.-T., and
Müller, E., “Neutrino heating, convection, and the mechanism of
Type-II supernova explosions”, Astron.
Astrophys., 306, 167-198,
(1996).
|
|
134 |
Jenet, F.A., and
Prince, T.A., “Detection of variable frequency signals using a fast
chirp transform”, Phys. Rev. D,
62, 122001-1-10, (2000). Related
online version (cited on 7 December 2000):
http://arXiv.org/abs/gr-qc/0012029.
|
|
135 |
Jones, P.B., “Bulk
viscosity of neutron-star matter”, Phys. Rev.
D, 64, 084003-1-7, (2001).
|
|
136 |
Jones, P.B., “Comment
on “Gravitational radiation instability in hot young neutron
stars””, Phys. Rev. Lett.,
86, 1384, (2001).
|
|
137 |
Kato, M., and Hachisu,
I., “A new estimation of mass accumulation efficiency in helium
shell flashes toward Type Ia supernova explosions”, Astrophys. J. Lett., 513, L41-L44, (1999). Related online version
(cited on 8 January 1999):
http://arXiv.org/abs/astro-ph/9901080.
|
|
138 |
Kifonidis,
K., Plewa, T., Scheck, L., Janka, H.-T., and Müller, E.,
“Non-Spherical Core-Collapse Supernovae II. Late-Time Evolution of
Globally Anisotropic Neutrino-Driven Explosions and Implications
for SN 1987A”, Astron. Astrophys.,
submitted, (2005). Related online version (cited on 21 December
2005):
http://arXiv.org/abs/astro-ph/0511369.
|
|
139 |
King, A.R., and Lasota,
J.-P., “Spin evolution and magnetic fields in cataclysmic
variables”, Astrophys. J.,
378, 674-681, (1991).
|
|
140 |
Kobayashi, S.,
and Mészáros, P., “Gravitational radiation from gamma-ray burst
progenitors”, Astrophys. J.,
589, 861-870, (2003). Related online
version (cited on 9 October 2002):
http://arXiv.org/abs/astro-ph/0210211.
|
|
141 |
Kobayashi, S.,
and Mészáros, P., “Polarized Gravitational Waves from Gamma-Ray
Bursts”, Astrophys. J., 585, L89-L92, (2003).
|
|
142 |
Kormendy, J.,
“Supermassive Black Holes in Disk Galaxies”, in Funes, J.G., and
Corsini, E.M., eds., Galaxy Disks and Disk
Galaxies, Proceedings of a conference sponsored by the
Vatican Observatory, held at the Pontifical Gregorian University in
Rome, Italy, 12-16 June 2000, vol. 230 of ASP Conference Series,
247-256, (Astronomical Society of the Pacific, San Francisco,
U.S.A., 2001).
|
|
143 |
Kotake, K.,
Katsuhiko, S., and Keitaro, T., “Explosion Mechanism, Neutrino
Burst, and Gravitational Wave in Core-Collapse Supernovae”,
Rep. Prog. Phys., submitted, (2005).
Related online version (cited on 21 December 2005):
http://arXiv.org/abs/astro-ph/0509456.
|
|
144 |
Kotake, K., Yamada,
S., and Sato, K., “Gravitational radiation from axisymmetric
rotational core collapse”, Phys. Rev.
D, 68, 044023, (2003).
|
|
145 |
Kotake, K.,
Yamada, S., Sato, K., Sumiyoshi, K., Ono, H., and Suzuki, H.,
“Gravitational radiation from rotational core collapse: Effects of
magnetic fields and realistic equations of state”, Phys. Rev. D, 69,
124004-1-11, (2004).
|
|
146 |
Lai, D., “Secular bar-mode
evolution and gravitational waves from neutron stars”, in
Centrella, J.M., ed., Astrophysical Sources
for Ground-based Gravitational Wave Detectors, Philadelphia,
Pennsylvania, USA, 30 October - 1 November 2000, vol. 575 of AIP
Conference Proceedings, 246-257, (American Institute of Physics,
Melville, U.S.A., 2001).
|
|
147 |
Lai, D., and Goldreich, P.,
“Growth of perturbations in gravitational collapse and accretion”,
Astrophys. J., 535, 402-411, (2000). Related online version
(cited on 25 June 1999):
http://arXiv.org/abs/astro-ph/9906400.
|
|
148 |
Lai, D., and Shapiro,
S.L., “Gravitational radiation from rapidly rotating nascent
neutron stars”, Astrophys. J.,
442, 259-272, (1995). Related online
version (cited on 17 August 1994):
http://arXiv.org/abs/astro-ph/9408053.
|
|
149 |
Leaver, E.W., “An
analytic representation for the quasi-normal modes of Kerr black
holes”, Proc. R. Soc. London, Ser. A,
402, 285-298, (1985).
|
|
150 |
Liebendörfer, M.,
Messer, O.E.B., Mezzacappa, A., Bruenn, S.W., Cardall, C.Y., and
Thielemann, F.-K., “A finite difference representation of neutrino
radiation hydrodynamics for spherically symmetric general
relativistic supernova simulations”, Astrophys. J. Suppl. Ser., 150, 263-316, (2004).
|
|
151 |
Lindblom,
L., and Owen, B.J., “Effect of hyperon bulk viscosity on
neutron-star r-modes”, Phys. Rev. D,
65, 063006-1-15, (2002). Related
online version (cited on 25 October 2001):
http://arXiv.org/abs/astro-ph/0110558.
|
|
152 |
Lindblom, L.,
Owen, B.J., and Morinsk, S.M., “Gravitational radiation instability
in hot young stars”, Phys. Rev. Lett.,
80, 4843-4846, (1998). Related online
version (cited on 13 March 1998):
http://arXiv.org/abs/gr-qc/9803053.
|
|
153 |
Lindblom, L.,
Tohline, J.E., and Vallisneri, M., “Nonlinear evolution of the
r-modes in neutron stars”,
Phys. Rev. Lett., 86, 1152-1155, (2001). Related online version
(cited on 31 October 2000):
http://arXiv.org/abs/astro-ph/0010653.
|
|
154 |
Lindblom, L.,
Tohline, J.E., and Vallisneri, M., “Numerical evolutions of
nonlinear r-modes in neutron stars”,
Phys. Rev. D, 65, 084039-1-15, (2002). Related online version
(cited on 20 September 2001):
http://arXiv.org/abs/astro-ph/0109352.
|
|
155 |
Liu, Y.T., “Dynamical
instability of new-born neutron stars as sources of gravitational
radiation”, Phys. Rev. D, 65, 124003-1-14, (2002). Related online version
(cited on 21 September 2001):
http://arXiv.org/abs/gr-qc/0109078.
|
|
156 |
Liu, Y.T., and Lindblom,
L., “Models of rapidly rotating neutron stars: remnants of
accretion-induced collapse”, Mon. Not. R.
Astron. Soc., 324, 1063-1073,
(2001). Related online version (cited on 9 December
2000):
http://arXiv.org/abs/astro-ph/0012198.
|
|
157 |
Loeb, A., and Rasio,
F.A., “Collapse of primordial gas clouds and the formation of
quasar black holes”, Astrophys. J.,
432, 52-61, (1994). Related online
version (cited on 16 January 1994):
http://arXiv.org/abs/astro-ph/9401026.
|
|
158 |
Loveridge,
L.C., “Gravitational waves from a pulsar kick caused by neutrino
conversions”, Phys. Rev. D, 69, 024008,
(2004).
|
|
159 |
Macchetto,
F.D., “Supermassive black holes and galaxy morphology”,
Astrophys. Space Sci., 269, 269-291, (1999). Related online version
(cited on 5 October 1999):
http://arXiv.org/abs/astro-ph/9910089.
|
|
160 |
MacFadyen,
A.I., and Woosley, S.E., “Collapsars: Gamma-Ray Bursts and
Explosions in “Failed Supernovae””, Astrophys. J., 524,
262-289, (1999).
|
|
161 |
Maiolino, R.,
Vanzi, L., Mannucci, F., Cresci, G., Ghinassi, F., and
Della Valle, M., “Discovery of two infrared supernovae: a new
window on the SN search”, Astron.
Astrophys., 389, 84-92, (2002).
|
|
162 |
Managan, R.A., “On
the secular instability of axisymmetric rotating stars to
gravitational radiation reaction”, Astrophys.
J., 294, 463-473, (1985).
|
|
163 |
Marck, J.-A., and
Bonazzola, S., “Gravitational radiation from three-dimensional
gravitational stellar core collapse”, in D’Inverno, R., ed.,
Approaches to Numerical Relativity,
Proceedings of the International Workshop on Numerical Relativity,
Southampton, England, 16-20 December 1991, 247, (Cambridge
University Press, Cambridge, U.K., 1992).
|
|
164 |
Max Planck Institute for
Astrophysics, “MPA Hydro Gang Homepage”, project homepage. URL
(cited on 17 April 2002):
http://www.mpa-garching.mpg.de/Hydro/index.shtml. url
updated in 2006 revision.
|
|
165 |
Max Planck Institute
for Astrophysics, “General relativistic simulations of rotational
supernova collapse”, project homepage, (2002). URL (cited on 3 July
2002):
http://www.mpa-garching.mpg.de/rel_hydro/axi_core_collapse/index.shtml.
url updated in 2006 revision.
|
|
166 |
Mayle, R., and Wilson,
J.R., “Supernovae from collapse of oxygen-magnesium-neon cores”,
Astrophys. J., 334, 909-926, (1988).
|
|
167 |
Mezzacappa,
A., Calder, A.C., Bruenn, S.W., Blondin, J.M., Guidry, M.W.,
Strayer, M.R., and Umar, A.S., “The interplay between proto-neutron
star convection and neutrino transport in core collapse
supernovae”, Astrophys. J.,
493, 848-862, (1998). Related online
version (cited on 18 September 1997):
http://arXiv.org/abs/astro-ph/9709184.
|
|
168 |
Mezzacappa,
A., Calder, A.C., Bruenn, S.W., Blondin, J.M., Guidry, M.W.,
Strayer, M.R., and Umar, A.S., “An investigation of neutrino-driven
convection and the core collapse supernova mechanism using
multigroup neutrino transport”, Astrophys.
J., 495, 911-926, (1998).
Related online version (cited on 18 September 1997):
http://arXiv.org/abs/astro-ph/9709188.
|
|
169 |
Misner, C.W., Thorne,
K.S., and Wheeler, J.A., Gravitation,
(Freeman, New York, U.S.A., 1973).
|
|
170 |
Mönchmeyer,
R., Schäfer, G., Müller, E., and Kates, R.E., “Gravitational waves
from the collapse of rotating stellar cores”, Astron. Astrophys., 246, 417-440, (1991).
|
|
171 |
Müller, E.,
“Gravitational radiation from collapsing rotating stellar cores”,
Astron. Astrophys., 114, 53-59, (1982).
|
|
172 |
Müller, E.,
“Gravitational waves from core collapse supernovae”, in Marck,
J.-A., and Lasota, J.-P., eds., Relativistic
Gravitation and Gravitational Radiation, Proceedings of the
Les Houches School of Physics, held in Les Houches, Haute Savoie,
26 September - 6 October, 1995, Cambridge Contemporary
Astrophysics, 273-308, (Cambridge University Press, Cambridge,
U.K., 1997).
|
|
173 |
Müller, E.,
“Simulation of astrophysical fluid flow”, in LeVeque, R.J.,
Mihalas, D., Dorfi, E.A., and Müller, E., eds., Computational Methods for Astrophysical Fluid
Flow, Lecture Notes 1997 of the Swiss Society for Astronomy
and Astrophysics (SSAA), held March 3-8, 1997 in Les Diablerets,
Switzerland, vol. 27 of Saas-Fee Advanced Courses, 343-494,
(Springer, Berlin, Germany; New York, U.S.A., 1998).
|
|
174 |
Müller, E., and
Hillebrandt, W., “The collapse of rotating stellar cores”,
Astron. Astrophys., 103, 358-366, (1981).
|
|
175 |
Müller, E.,
Hillebrandt, W., and Rozyczka, M., “Stellar Collapse - Adiabatic
hydrodynamics and shock wave propagation”, Astron. Astrophys., 81, 288-292, (1980).
|
|
176 |
Müller, E., and
Janka, H.-T., “Gravitational radiation from convective
instabilities in Type II supernova explosions”, Astron. Astrophys., 317, 140-163, (1997).
|
|
177 |
Müller, E.,
Rampp, M., Buras, R., Janka, H.-T., and Shoemaker, D.H., “Toward
Gravitational Wave Signals from Realistic Core-Collapse Supernova
Models”, Astrophys. J., 603, 221-230, (2004).
|
|
178 |
Nadyozhin,
D.K., “Physical Properties of SNe IIP Derived from a Comparison of
Theoretical Models with Observations”, Astron. Astrophys., submitted, (2002). Related
online version (cited on 09 January 2006):
http://www.mpa-garching.mpg.de/mpa/publications/preprints/pp2002/pp2002-en.html.
|
|
179 |
Nakamura, T.,
“General relativistic collapse of axially symmetric stars leading
to the formation of rotating black holes”, Prog. Theor. Phys., 65, 1876-1890, (1981).
|
|
180 |
Nakamura, T.,
“General Relativistic Collapse of Accreting Neutron Stars with
Rotation”, Prog. Theor. Phys., 70,
1144-1147, (1983).
|
|
181 |
NASA/ESA, “Laser Interferometer
Space Antenna”, project homepage. URL (cited on 4 October
2002):
http://lisa.jpl.nasa.gov.
|
|
182 |
National
Astronomical Observatory, “TAMA Project”, project homepage. URL
(cited on 4 October 2002):
http://tamago.mtk.nao.ac.jp/.
|
|
183 |
Nazin, S.N., and
Postnov, K.A., “High neutron star birth velocities and
gravitational radiation during supernova explosions”, Astron. Astrophys., 317, L79-L81, (1997). Related online version
(cited on 15 January 1997):
http://arXiv.org/abs/astro-ph/9701073.
|
|
184 |
New, K.C.B., Centrella,
J.M., and Tohline, J.E., “Gravitational waves from long-duration
simulations of the dynamical bar instability”, Phys. Rev. D, 62,
064019-1-16, (2000). Related online version (cited on 30 November
1999):
http://arXiv.org/abs/astro-ph/9911525.
|
|
185 |
New, K.C.B., and
Shapiro, S.L., “Evolution of differentially rotating supermassive
stars to the onset of bar instability”, Astrophys. J., 548,
439-446, (2001). Related online version (cited on 9 October
2000):
http://arXiv.org/abs/astro-ph/0010172.
|
|
186 |
New, K.C.B., and
Shapiro, S.L., “The formation of supermassive black holes and the
evolution of supermassive stars”, Class.
Quantum Grav., 18, 3965-3976,
(2001). Related online version (cited on 6 September
2000):
http://arXiv.org/abs/astro-ph/0009095.
|
|
187 |
Nomoto, K., and
Kondo, Y., “Conditions for accretion-induced collapse of white
dwarfs”, Astrophys. J. Lett.,
367, L19-L22, (1991).
|
|
188 |
Novikov, I.D.,
“Gravitational radiation from a star collapsing into a disk”,
Sov. Astron., 19, 398, (1975).
|
|
189 |
Oshea, B.W.,
Norman M., personal communication, (2005).
|
|
190 |
Ott, C.D., Burrows, A.,
Livne, E., and Walder, R., “Gravitational Waves from Axisymmetric,
Rotating Stellar Core Collapse”, Astrophys.
J., 600, 834-864, (2004).
|
|
191 |
Ou, S., Tohline, J.E., and
Lindblom, L., “Supernovae and the nuclear equation of state at high
densities”, Astrophys. J.,
617, 490-499, (2004).
|
|
192 |
Pickett, B.K.,
Durisen, R.H., and Davis, G., “The dynamic stability of rotating
protostars and protostellar disks. I. The effects of the angular
momentum distribution”, Astrophys. J.,
458, 714-738, (1996).
|
|
193 |
Piran, T., and
Stark, R.F., “Numerical relativity, rotating gravitational
collapse, and gravitational radiation”, in Centrella, J.M., ed.,
Dynamical Spacetimes and Numerical
Relativity, Proceedings of a workshop
held at Drexel University, October 7-11, 1985, 40-73, (Cambridge
University Press, Cambridge, U.K.; New York, U.S.A., 1986).
|
|
194 |
Podsiadlowski, P., Joss, P.C., and Hsu,
J.J.L., “Presupernova evolution in massive interacting binaries”,
Astrophys. J., 391, 246-264, (1992).
|
|
195 |
Popham, R., Woosley,
S.E., and Fryer, C.L., “Hyperaccreting Black Holes and Gamma-Ray
Bursts”, Astrophys. J., 518, 356-374, (1999).
|
|
196 |
Proga, D.,
MacFadyen, A.I., Armitage, P.J., and Begelman, M.C., “Axisymmetric
Magnetohydrodynamic Simulations of the Collapsar Model for
Gamma-Ray Bursts”, Astrophys. J.
Lett., 599, L5-L8, (2003).
|
|
197 |
Rampp, M., and
Janka, H.-T., “Radiation hydrodynamics with neutrinos: Variable
Eddington factor method for core-collapse supernova simulations”,
Astron. Astrophys., 396, 361-392, (2002). Related online version
(cited on 7 March 2002):
http://arXiv.org/abs/astro-ph/0203101.
|
|
198 |
Rampp, M., Müller,
E., and Ruffert, M., “Simulations of non-axisymmetric rotational
core collapse”, Astron. Astrophys.,
332, 969-983, (1998). Related online
version (cited on 11 November 1997):
http://arXiv.org/abs/astro-ph/9781112.
|
|
199 |
Rees, M.J.,
“Astrophysical Evidence for Black Holes”, in Wald, R.M., ed.,
Black Holes and Relativistic Stars, Proceedings of the Symposium
dedicated to the memory of Subrahmanyan Chandrasekhar, held in
Chicago, December 14-15, 1996, 79-101, (University of Chicago
Press, Chicago, U.S.A.; London, U.K., 1998).
|
|
200 |
Rezzolla, L.,
“Relativistic Astrophysics movies at SISSA”, personal homepage,
SISSA / ISAS. URL (cited on 4 October 2002):
http://www.sissa.it/~rezzolla/movies.html.
|
|
201 |
Rezzolla, L.,
Lamb, F.K., Marković, D., and Shapiro, S.L., “Properties of
r modes in rotating magnetic neutron
stars. I. Kinematic secular effects and magnetic evolution”,
Phys. Rev. D, 64, 104013-1-12, (2001). Related online version
(cited on 17 July 2001):
http://arXiv.org/abs/gr-qc/0107061.
|
|
202 |
Rezzolla, L.,
Lamb, F.L., Markovic, D., and Shapiro, S.L., “Properties of
r modes in rotating magnetic neutron
stars. II. Evolution of the r modes
and stellar magnetic field”, Phys. Rev.
D, 64, 104014-1-13, (2001).
Related online version (cited on 17 July 2001):
http://arXiv.org/abs/gr-qc/0107062.
|
|
203 |
Ruffini, R., and
Wheeler, J.A., “Relativistic Cosmology from Space Platforms”, in
Hardy, V., and H. Moore, H., eds., Proceedings of the Conference on Space Physics,
45-174, (ESRO, Paris, France, 1971).
|
|
204 |
Saenz, R.A., and
Shapiro, S.L., “Gravitational radiation from stellar collapse -
Ellipsoidal models”, Astrophys. J.,
221, 286-303, (1978).
|
|
205 |
Saenz, R.A., and
Shapiro, S.L., “Gravitational and neutrion radiation from stellar
core collapse - Improved ellipsoidal model calculations”,
Astrophys. J., 229, 1107-1125, (1979).
|
|
206 |
Saenz, R.A., and
Shapiro, S.L., “Gravitational radiation from stellar core collapse.
III - Damped ellipsoidal oscillations”, Astrophys. J., 244,
1033-1038, (1981).
|
|
207 |
Saijo, M., “The
Collapse of Differentially Rotating Supermassive Stars: Conformally
Flat Simulations”, Astrophys. J.,
615, 866-879, (2004).
|
|
208 |
Saijo, M., Baumgarte,
T.W., Shapiro, S.L., and Shibata, M., “Collapse of a rotating
supermassive star to a supermassive black hole: Post-Newtonian
simulations”, Astrophys. J.,
569, 349-361, (2002). Related online
version (cited on 6 February 2002):
http://arXiv.org/abs/astro-ph/0202112.
|
|
209 |
Saijo, M., Shibata, M.,
Baumgarte, T.W., and Shapiro, S.L., “Dynamical bar instability in
rotating stars: effect of general relativity”, Astrophys. J., 548,
919-931, (2001). Related online version (cited on 10 October
2000):
http://arXiv.org/abs/astro-ph/0010201.
|
|
210 |
Salpeter,
E.E., “Energy and pressure of a zero-temperature plasma”,
Astrophys. J., 134, 669-682, (1961).
|
|
211 |
Sanders, R.H., “The
effects of stellar collisions in dense stellar systems”,
Astrophys. J., 162, 791-809, (1970).
|
|
212 |
Scheck, L., Plewa,
T., Janka, H.-T., Kifonidis, K., and Müller, E., “Pulsar Recoil by
Large-Scale Anisotropies in Supernova Explosions”, Phys. Rev. Lett., 92,
011103, (2004).
|
|
213 |
Schenk, A.K.,
Arras, P., Flanagan, É.É., Teukolsky, S.A., and Wasserman, I.,
“Nonlinear mode coupling in rotating stars and the r-mode instability in neutron stars”, Phys. Rev. D, 65,
024001-1-43, (2002). Related online version (cited on 23 January
2001):
http://arXiv.org/abs/gr-qc/0101092.
|
|
214 |
Schutz, B.F.,
“Gravitational Wave Astronomy”, Class.
Quantum Grav., 16, A131-A156,
(1999). Related online version (cited on 9 November
1999):
http://arXiv.org/abs/gr-qc/9911034.
|
|
215 |
Seidel, E., and
Moore, T., “Gravitational radiation from realistic relativistic
stars: Odd-parity fluid perturbations”, Phys.
Rev. D, 35, 2287-2296, (1987).
|
|
216 |
Seidel, E., and
Moore, T., “Gravitational radiation from perturbations of stellar
core collapse models”, in Evans, C.R., Finn, L.S., and Hobill,
D.W., eds., Frontiers in Numerical
Relativity, 146-162, (Cambridge
University Press, Cambridge, U.K.; New York, U.S.A., 1988).
|
|
217 |
Sekiguchi,
Y., and Shibata, M., “New criterion for direct black hole formation
in rapidly rotating stellar collapse”, Phys.
Rev. D, 70, 084005, (2004).
|
|
218 |
Shapiro, S.L.,
“Gravitational radiation from stellar collapse - The initial
burst”, Astrophys. J., 214, 566-575, (1977).
|
|
219 |
Shapiro, S.L.,
and Lightman, A.P., “Rapidly rotating, post-Newtonian neutron
stars”, Astrophys. J., 207, 263-278, (1976).
|
|
220 |
Shapiro, S.L., and
Teukolsky, S.A., “Gravitational collapse of supermassive stars to
black holes - Numerical solution of the Einstein equations”,
Astrophys. J., 234, L177-L181, (1979).
|
|
221 |
Shapiro, S.L., and
Teukolsky, S.A., Black Holes, White Dwarfs,
and Neutron Stars, (Wiley, New York, U.S.A., 1983).
|
|
222 |
Shibata,
M., “Axisymmetric Simulations of Rotating Stellar Collapse in Full
General Relativity - Criteria for Prompt Collapse to Black Holes
-”, Prog. Theor. Phys., 104, 325-358, (2000). Related online version
(cited on 19 July 2000):
http://arXiv.org/abs/gr-qc/0007049.
|
|
223 |
Shibata, M.,
Baumgarte, T.W., and Shapiro, S.L., “The bar-mode instability in
differentially rotating neutron stars: Simulations in full general
relativity”, Astrophys. J.,
542, 453-463, (2000). Related online
version (cited on 18 May 2000):
http://arXiv.org/abs/astro-ph/0005378.
|
|
224 |
Shibata, M.,
Baumgarte, T.W., and Shapiro, S.L., “Stability and collapse of
rapidly rotating, supramassive neutron stars: 3D simulations in
general relativity”, Phys. Rev. D,
61, 044012-1-11, (2000). Related
online version (cited on 16 November 1999):
http://arXiv.org/abs/astro-ph/9911308.
|
|
225 |
Shibata, M., and
Karino, S., “Numerical evolution of secular bar-mode instability
induced by gravitational radiation reaction in rapidly rotating
neutron stars”, Phys. Rev. D,
70, 084022-1-15, (2004).
|
|
226 |
Shibata, M.,
Karino, S., and Eriguchi, Y., “Dynamical instability of
differentially rotating stars”, Mon. Not. R.
Astron. Soc., 334, L27-L32,
(2002). Related online version (cited on 6 June 2002):
http://arXiv.org/abs/gr-qc/0206002.
|
|
227 |
Shibata, M.,
Karino, S., and Eriguchi, Y., “Dynamical bar-mode instability of
differentially rotating stars: effects of equations of state and
velocity profiles”, Mon. Not. R. Astron.
Soc., 343, 619-626, (2003).
|
|
228 |
Shibata, M., and
Shapiro, S.L., “Collapse of a rotating supermassive star to a
supermassive black hole: Fully relativistic simulations”,
Astrophys. J. Lett., 572, L39-L43, (2002). URL (cited on 07 May
2002):
http://arXiv.org/abs/astro-ph/0205091.
|
|
229 |
Shibata, M.,
Shapiro, S.L., and Uryu, K., “Equilibrium and stability of
supermassive stars in binary systems”, Phys.
Rev. D, 64, 24004-1-14, (2001).
Related online version (cited on 25 April 2001):
http://arXiv.org/abs/astro-ph/0104408.
|
|
230 |
Shibata, M., and
Yu-ichirou, S., “Gravitational waves from axisymmetric rotating
stellar core collapse to a neutron star in full general
relativity”, Phys. Rev. D,
69, 084024-1-16, (2004).
|
|
231 |
Smith, S., Houser,
J.L., and Centrella, J.M., “Simulations of nonaxisymmetric
instability in a rotating star: A comparison between Eulerian and
Smooth Particle Hydrodynamics”, Astrophys.
J., 458, 236-256, (1996).
Related online version (cited on 9 October 1995):
http://arXiv.org/abs/gr-qc/9510014.
|
|
232 |
Spruit, H.C., “Dynamo
action by differential rotation in a stably stratified stellar
interior”, Astron. Astrophys.,
381, 923-932, (2002).
|
|
233 |
Stark, R.F., and
Piran, T., “Gravitational wave emission from rotating gravitational
collapse”, Phys. Rev. Lett.,
55, 891-894, (1985).
|
|
234 |
Starrfield,
S., Timmes, F.X., Hix, W.R., Sion, E.M., Sparks, W.M., and Dwyer,
S.J., “Surface Hydrogen-burning Modeling of Supersoft X-ray
Binaries: Are they Type Ia Supernovae Progenitors?”, Astrophys. J., 612,
L53-L56, (2004).
|
|
235 |
Stergioulas, N., Apostolatos, T.A., and Font,
J.A., “Non-linear pulsations in differentially rotating neutron
stars: mass-shedding-induced damping and splitting of the
fundamental mode”, Mon. Not. R. Astron.
Soc., 352, 1089-1101, (2004).
|
|
236 |
Stergioulas, N., and Font, J.A., “Nonlinear
r-modes in rapidly rotating
relativistic stars”, Phys.
Rev. Lett., 86, 1148-1151, (2001). Related online version
(cited on 31 July 2000):
http://arXiv.org/abs/gr-qc/0007086.
|
|
237 |
Swesty, F.D.,
Lattimer, J.M., and Myra, E.S., “The role of the equation of state
in the ‘prompt’ phase of type II supernovae”, Astrophys. J., 425,
195-204, (1994).
|
|
238 |
Symbalisty, E.M.D., “Magnetorotational iron core
collapse”, Astrophys. J., 285, 729-746, (1984).
|
|
239 |
Tassoul, J.-L.,
Theory of Rotating Stars, (Princeton
University Press, Princeton, U.S.A., 1978).
|
|
240 |
Thompson,
T.A., Burrows, A., and Pinto, P.A., “Shock breakout in
core-collapse supernovae and its neutrino signature”, Astrophys. J., 592,
434-456, (2003). URL (cited on 10 November 2002):
http://arXiv.org/abs/astro-ph/0211194.
|
|
241 |
Thorne, K.S.,
“Multipole expansion of gravitational radiation”, Rev. Mod. Phys., 52,
299-340, (1980).
|
|
242 |
Thorne, K.S.,
“Gravitational Radiation”, in Hawking, S.W., and Israel, W., eds.,
Three Hundred Years of Gravitation, 330-458, (Cambridge
University Press, Cambridge, U.K.; New York, U.S.A., 1987).
|
|
243 |
Thorne, K.S.,
“Gravitational radiation”, in Böhringer, H., Morfill, G.E., and
Trümper, J.E., eds., 17th Texas Symposium on
Relativistic Astrophysics and Cosmology, vol. 759 of Annals
of the New York Academy of Sciences, 127-152, (New York Academy of
Sciences, New York, U.S.A., 1995).
|
|
244 |
Thorne, K.S.,
“Gravitational Waves from Compact Bodies”, in van Paradijs, J.,
van den Heuvel, E.P.J., and Kuulkers, E., eds., Compact Stars in Binaries, Proceedings of the
165th Symposium of the International Astronomical Union, held in
The Hague, the Netherlands, August 15-19, 1994, vol. 165 of IAU
Symposia, 153-184, (Kluwer Academic Publishers, Dordrecht,
Netherlands; Boston, U.S.A., 1996). Related online version (cited
on 30 June 1995):
http://arXiv.org/abs/gr-qc/9506084.
|
|
245 |
Thuan, T.X., and
Ostriker, J.P., “Gravitational radiation from stellar collapse”,
Astrophys. J. Lett., 191,
L105-L107, (1974).
|
|
246 |
Tohline, J.E.,
“The collapse of rotating stellar cores - Equilbria between white
dwarf and neutron star densities”, Astrophys.
J., 285, 721-728, (1984).
|
|
247 |
Tohline, J.E.,
and Hachisu, I., “The breakup of self-gravitating rings, tori, and
thick accretion disks”, Astrophys. J.,
361, 394-407, (1990).
|
|
248 |
Toman, J., Imamura,
J.N., Pickett, B.K., and Durisen, R.H., “Nonaxisymmetric dynamic
instabilities of rotating polytropes. I. The Kelvin modes”,
Astrophys. J., 497, 370-387, (1998).
|
|
249 |
Turner, M.S., and
Wagoner, R.V., “Gravitational radiation from slowly-rotating
supernovae - Preliminary results”, in Smarr, L.L., ed.,
Sources of Gravitational Radiation,
Proceedings of the Battelle Seattle Workshop, July 24 - August 4,
1978, 383-407, (Cambridge University Press, Cambridge, U.K., 1979).
|
|
250 |
van Putten,
M.H.P.M., “Gravitational Wave Frequencies and Energies in
Hypernovae”, Astrophys. J.,
583, 374-378, (2003).
|
|
251 |
van Putten,
M.H.P.M., and Levinson, A., “Theory and astrophysical consequences
of a magnetized torus around a rapidly rotating black hole”,
Astrophys. J., 584, 937-953, (2003). URL (cited on 12 December
2002):
http://arXiv.org/abs/astro-ph/0212297.
|
|
252 |
Villain, L., Pons,
J.A., Cerdá-Durán, P., and Gourgoulhon, E., “Evolutionary sequences
of rotating protoneutron stars”, Astron.
Astrophys., 418, 283-294,
(2004).
|
|
253 |
Walder, R.,
Burrows, A., Ott, C.D., Livne, E., Lichtenstadt, I., and Jarrah,
M., “Anisotropies in the Neutrino Fluxes and Heating Profiles in
Two-dimensional, Time-dependent, Multigroup Radiation Hydrodynamics
Simulations of Rotating Core-Collapse Supernovae”, Astrophys. J., 626,
317-332, (2005).
|
|
254 |
Watts, A.L., Andersson,
N., and Jones, D.I., “The Nature of Low T/|W| Dynamical Instabilities in Differentially
Rotating Stars”, Astrophys. J. Lett.,
618, L37-L40, (2005).
|
|
255 |
Wheeler, J.C., Yi,
I., Höflich, P., and Wang, L., “Asymmetric Supernovae, Pulsars,
Magnetars, and Gamma-Ray Bursts”, Astrophys.
J., 537, 810-823, (2000).
|
|
256 |
Wickramasinghe, D.T., and Ferrario, L.,
“Magnetism in Isolated and Binary White Dwarfs”, Publ. Astron. Soc. Pac., 112, 873-924, (2000).
|
|
257 |
Wilson, J.R.,
“title missing”, in Centrella, J.M., LeBlanc, J.M., and Bowers,
J.L., eds., Numerical Astrophysics,
Proceedings of a symposium in honor of James R. Wilson, held at the
University of Illinois in October, 1982, 422-434, (Jones and
Barlett, Boston, U.S.A., 1985).
|
|
258 |
Wilson, J.R., and
Mayle, R., “Convection in core collapse supernovae”, Phys. Rep., 163,
63-78, (1988).
|
|
259 |
Wilson, J.R., Mayle,
R., Woosley, S.E., and Weaver, T.A., “Stellar Core Collapse and
Supernovae”, Ann. N.Y. Acad. Sci.,
470, 267-293, (1986).
|
|
260 |
Woodward, J.,
Tohline, J.E., and Hachisu, I., “The stability of thick,
self-gravitating disks in protostellar systems”, Astrophys. J., 420,
247-267, (1994).
|
|
261 |
Woosley, S.E., “Gamma-Ray
Bursts From Stellar Mass Accretion Disks Around Black Holes”,
Astrophys. J., 405, 273-277, (1993).
|
|
262 |
Woosley, S.E.,
“Gamma-ray bursts from stellar mass accretion disks around black
holes”, Astrophys. J., 405, 273-277, (1993).
|
|
263 |
Woosley, S.E., and
Baron, E., “The collapse of white dwarfs to neutron stars”,
Astrophys. J., 391, 228-235, (1992).
|
|
264 |
Yamada, S., and Sato,
K., “Gravitational radiation from rotational collapse of a
supernova core”, Astrophys. J.,
450, 245-252, (1995).
|
|
265 |
Yooun, S.C., and
Langer, N., “Evolution of rapidly rotating metal-poor massive stars
towards gamma-ray bursts”, Astron.
Astrophys., 443, 643-648,
(2005).
|
|
266 |
Young, P.A., Fryer,
C.L., Hungerford, A., Arnett, D., Rockefeller, G., Timmes, F.X.,
Voit, B., Meakin, C., and Eriksen, K.A., “Constraints on the
Progenitor of Cassiopeia A”, Astrophys. J.,
accepted, (2005). Related online version (cited on 21 December
2005):
http://arXiv.org/abs/astro-ph/0511806.
|
|
267 |
Yu-ichirou, S., and Shibata, M.,
“Axisymmetric collapse simulations of rotating massive stellar
cores in full general relativity: Numerical study for prompt black
hole formation”, Phys. Rev.
D, 71,
084013-1-30, (2005).
|
|
268 |
Yungelson,
L.R., and Livio, M., “Type Ia Supernovae: An Examination of
Potential Progenitors and the Redshift Distribution”, Astrophys. J., 497,
168-177, (1998). Related online version (cited on 18 November
1997):
http://arXiv.org/abs/astro-ph/9711201.
|
|
269 |
Zanotti, O.,
Rezzolla, L., and Font, J.A., “Quasi-periodic accretion and
gravitational waves from oscillating “toroidal neutron stars”
around a Schwarzschild black hole”, Mon. Not.
R. Astron. Soc., 341, 832-848, (2003).
|
|
270 |
Zel’dovich,
Y.B., and Novikov, I.D., Relativistic
Astrophysics, vol. 1, (University of Chicago Press,
Chicago, U.S.A., 1971).
|
|
271 |
Zwerger, T., and
Müller, E., “Dynamics and gravitational wave signature of
axisymmetric rotational core collapse”, Astron. Astrophys., 320, 209-227, (1997).
|
