Published August 1, 2012
| Version 3168
Journal article
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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
Description
MESA models computed for comparison with Victoria models.
Files
Mpoor_fh.zip
Files
(4.6 kB)
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Additional details
Related works
- Is documented by
- 10.1088/0004-637X/755/1/15 (DOI)
References
- VandenBerg et al. (2012)