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Abundances and kinematics of field halo and disk stars

✍ Scribed by J.P. Fulbright


Publisher
Elsevier Science
Year
2001
Tongue
English
Weight
129 KB
Volume
688
Category
Article
ISSN
0375-9474

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## Abstract Sulphur is a volatile __Ξ±__ ‐element which is not locked into dust grains in the interstellar medium (ISM). Hence, its abundance does not need to be corrected for dust depletion when comparing the ISM to the stellar atmospheres. The abundance of sulphur in the photosphere of metal‐poor

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