Journal article Open Access

Models for Metal-poor Stars with Enhanced Abundances of C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti, in Turn, at Constant Helium and Iron Abundances

Aaron Dotter

MESA models computed for comparison with Victoria models.

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  • VandenBerg et al. (2012)

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Publication date:
August 1, 2012
DOI:
10.5281/zenodo.2598616

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10.5281/zenodo.2598616

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Astrophysical Journal: 755.
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10.1088/0004-637X/755/1/15
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