Pith. sign in

REVIEW

From Darkness To Light: The First Stars in the Universe

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv astro-ph/0110459 v1 pith:2YM2HEB2 submitted 2001-10-20 astro-ph

From Darkness To Light: The First Stars in the Universe

classification astro-ph
keywords firststarsbeenmassiveagesbasicconstrainingcosmic
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
Share X Bluesky LinkedIn Reddit HN
read the original abstract

Paramount among the processes that ended the cosmic `dark ages' must have been the formation of the first generation of stars (the so-called Population III). We summarize recent progress in constraining its nature, and we discuss the basic physical reasons for why the first stars might have been quite massive, possibly even very massive with M > 100 M_sun.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.