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An Ultra Metal-Poor Star Identified from Narrowband Photometry

43 点作者 SmkyMt大约 4 年前

6 条评论

wcoenen大约 4 年前
For those who don't know, "metal" doesn't actually mean metal in astronomy. They use the term to refer to any element that isn't hydrogen or helium.
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simonh大约 4 年前
What particularly surprises me about this is that the star is in our own galaxy. I&#x27;m used to the idea of seeing remnants from the early universe from observations of very distant galaxies, but of course then we&#x27;re seeing them as they were long ago. This is a second generation star that&#x27;s almost as old as the universe, but in our neighbourhood and we&#x27;re seeing it as it is &quot;now&quot; (or close enough).<p>I wonder where in the galaxy it&#x27;s located? Intuitively I&#x27;d expect such an object to survive longer if it were out in the rim or halo of the galaxy, in a more rarified region, but of course intuition on these things can be very misleading.
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qrybam大约 4 年前
&gt; Based on its chemical abundance pattern, we speculate that SPLUS J2104−0049 could be a bona fide second-generation star, formed from a gas cloud polluted by a single metal-free ~ 30M⊙ star
est31大约 4 年前
<a href="https:&#x2F;&#x2F;arxiv.org&#x2F;abs&#x2F;2105.04573" rel="nofollow">https:&#x2F;&#x2F;arxiv.org&#x2F;abs&#x2F;2105.04573</a>
spiritplumber大约 4 年前
Wonder if it means that it&#x27;s especially old, or it&#x27;s just the luck of the draw.
dvh大约 4 年前
Do metal-poor stars have terrestrial planets?
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