A stellar relic from the early Milky Way

Details A stellar relic from the early Milky Way A stellar relic from the early Milky Way

2002-11-13

arxiv.org/abs/astro-ph/0211274v1

Nature 419 (2002) 904-906

Astronomy and Astrophysics

Astrophysics

Offprint of Nature 419 (2002), 904-906 (issue 31 October 2002)

Scientific paper

10.1038/nature01142

The chemical composition of the most metal-deficient stars reflects the composition of the gas from which they formed. These old stars provide crucial clues to the star formation history and the synthesis of chemical elements in the early Universe. They are the local relics of epochs otherwise observable only at very high redshifts; if totally metal-free (``population III'') stars could be found, this would allow the direct study of the pristine gas from the Big Bang. Earlier searches for such stars found none with an iron abundance less than 1/10,000 that of the Sun, leading to the suggestion that low-mass stars could only form from clouds above a critical iron abundance. Here we report the discovery of a low-mass star with an iron abundance as low as 1/200,000 of the solar value. This discovery suggests that population III stars could still exist, that is, that the first generation of stars also contained long-lived low-mass objects. The previous failure to find them may be an observational selection effect.

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