Bibcode
DOI
Abia, C.; Rebolo, R.
Bibliographical reference
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 347, Dec. 1, 1989, p. 186-194.
Advertised on:
12
1989
Journal
Citations
173
Refereed citations
140
Description
The oxygen abundance has been determined by analysis of the O I infrared
triplet in 30 unevolved field stars of metallicities in the range Fe/H
abundance ratio between -0.2 and -3.5. The data show that the O/Fe
abundance ratio increases monotonically as metallicity decreases from
solar, reaching values in the range 1.0-1.2 at an Fe/H abundance ratio
of about -2. The results, when compared with those already published for
metal-deficient red giants, suggest that oxygen could have been depleted
in the latter. A discussion of the O/Fe abundance ratios in connection
with the chemical evolution of the Galaxy is also presented.