NDLI: Chemical Abundances of Metal-poor stars in Dwarf Galaxies

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Chemical Abundances of Metal-poor stars in Dwarf Galaxies

Content Provider	Scilit
Author	Venn, Kim A. Jablonka, Pascale Hill, Vanessa Starkenburg, Else Lemasle, Bertrand Shetrone, Matthew Irwin, Mike Norris, John Yong, David Gilmore, Gerry Salvadori, Stephania Skuladottir, Asa Tolstoy, Eline
Copyright Year	2015
Description	Stars in low-mass dwarf galaxies show a larger range in their chemical properties than those in the Milky Way halo. The slower star formation efficiency make dwarf galaxies ideal systems for testing nucleosynthetic yields. Not only are alpha-poor stars found at lower metallicities, and a higher fraction of carbon-enhanced stars, but we are also finding stars in dwarf galaxies that appear to be iron-rich. These are compared with yields from a variety of supernova predictions.
Related Links	https://www.cambridge.org/core/services/aop-cambridge-core/content/view/E409F9A519C7E635F5B9FB911C34F1DF/S1743921316000107a.pdf/div-class-title-chemical-abundances-of-metal-poor-stars-in-dwarf-galaxies-div.pdf
Ending Page	163
Page Count	5
Starting Page	159
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s1743921316000107
Journal	Proceedings of the International Astronomical Union
Issue Number	S317
Volume Number	11
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2015-08-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics Abundances Dwarf Local Group Stellar Content
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science

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