Super and massive AGB stars – III. Nucleosynthesis in metal-poor and very metal-poor stars – Z = 0.001 and 0.0001-Reference-Cited by-同舟云学术

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Super and massive AGB stars – III. Nucleosynthesis in metal-poor and very metal-poor stars – Z = 0.001 and 0.0001

Published:2014-04-27 Issue:1 Volume:441 Page:582-598
ISSN:1365-2966
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Doherty Carolyn L.,Gil-Pons Pilar,Lau Herbert H. B.,Lattanzio John C.,Siess Lionel,Campbell Simon W.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/441/1/582/13764853/stu571.pdf

Reference111 articles.

1. Origin of abundance inhomogeneity in globular clusters

2. Dynamical modeling of long-period variable star atmospheres

3. Helium in first and second-generation stars in globular clusters from spectroscopy of red giants

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