Here's a short (12 page) and pretty easy article from The Astrophysical Journal (2003), about end of life for massive stars. And why some would "directly" collapse (no big & bright supernova) into black holes.<p><a href="https://open.clemson.edu/cgi/viewcontent.cgi?article=1006&context=physastro_pubs" rel="nofollow">https://open.clemson.edu/cgi/viewcontent.cgi?article=1006&co...</a>
It's been a while since I crawled Wikipedia's rabbit hole on this - but I recall there being regions of the stellar "mass vs. metallicity" graph in which direct collapse to a black hole is the expected outcome.<p>Is there an astrophysicist in the house?
<p><pre><code> As many as 30 percent of such stars
may quietly collapse into black holes
no supernova required.
</code></pre>
where 'such' refers to 25 solar mass stars.<p>Is that a significant contribution to 'dark matter'?
Here is an article about some JWST data of the star.<p><a href="https://arxiv.org/abs/2309.16121" rel="nofollow">https://arxiv.org/abs/2309.16121</a>