[HN Gopher] Andromeda XXXV: The Faintest Dwarf Satellite of the ...
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Andromeda XXXV: The Faintest Dwarf Satellite of the Andromeda
Galaxy
Author : PaulHoule
Score : 40 points
Date : 2025-03-20 05:46 UTC (4 days ago)
(HTM) web link (iopscience.iop.org)
(TXT) w3m dump (iopscience.iop.org)
| merek wrote:
| This could have been an interesting article, but I couldn't get
| past the ridiculous captcha
| d_silin wrote:
| https://iopscience.iop.org/article/10.3847/2041-8213/adb433/...
| 0hijinks wrote:
| Here's an ArXiv version: https://arxiv.org/abs/2502.19516
| sega_sai wrote:
| I am not sure that it is that remarkable (for this website),
| given the _known_ faintest Milky Way 's satellites are ~ 100
| times fainter, and there probably ten-ish galaxies fainter than
| And XXXV around the MW.
| s1artibartfast wrote:
| What is the threshold for remark? I certainly wasn't aware
| there was a contest where only the faintest could be submitted?
| sega_sai wrote:
| I am not a policeman of what could be submitted, but some
| results are remarkable enough/interesting enough because they
| are record breakers or unusual in one way or another. This is
| run of the mill galaxy in Andromeda. And because Andromeda is
| quite far away the faintest galaxies we can detect there are
| in fact much brighter than what we can detect around the MW.
| s1artibartfast wrote:
| I guess I'm fundamentally pushing back on the idea that it
| has to be at the extreme end of a phenomenon to be
| interesting. I think the phenomenon of tiny satellite
| galaxies is interesting, full stop. far more remarkable
| than something being the smallest. Any distribution will
| have a smallest element, it follows from the distribution
| existing at all. Similarly, if satellite in orbit of
| Andromeda I don't see the value of bringing whataboutism
| into it.
| dredmorbius wrote:
| 1st 'graph of the related paper explains the significance:
|
| _Ultrafaint dwarf galaxies are critical probes of the
| properties of dark matter and the physical drivers of galaxy
| formation at very low mass scales. In the roughly two decades
| since their first discovery, tens of ultrafaint satellite
| galaxies of the Milky Way have been discovered. As individual
| systems, they are extremely dark matter dominated and most
| appear to have primarily early star formation that is impacted
| strongly by reionization._
|
| <https://iopscience.iop.org/article/10.3847/2041-8213/adb433/..
| .>
|
| To be fair, this is the _paper_ on which the article is
| presumably based rather than TFA itself, though I (as
| apparently others) was unable to read the linked source due to
| the indeed ridiculously stringent CAPTCHA.
|
| Obvious reasons why faint dwarf galaxies proximate to our own
| home galaxy might be more observable than even those of our
| nearest (large) galactic neighbour are obvious, and are a
| trivial tangent not worth elaboration.
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