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Results 1 - 4 of 4

Isochrones for Old (> 5 Gyr) Stars and Stellar Populations. I. Models for $-2.4 le$ [Fe/H] $le +0.6$, $0.25 le Y le 0.33$, and $-0.4 le$ [$α$Fe] $le +0.4$
- Volume 9, Issue 22 - article #40
- Don A. VandenBerg, Peter A. Bergbusch, Jason W. Ferguson, Bengt Edvardsson
- arXiv.org - Astrophysics - Volume: 2014, Issue: 5 Sep
- arXiv:1409.1283 [pdf, ps, other]
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
- Volume 7, Issue 33 - article #22
- Don A. VandenBerg, Peter A. Bergbusch, Aaron Dotter, Jason W. Ferguson, Georges Michaud, Jacques Richer, and Charles R. Proffitt
- The Astrophysical Journal - Volume: 755, Issue: 1
- Abstract References Full text PDF (1.43 MB) View as HTML
Stellar Models with Enhanced Abundances of C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti, in Turn, at Constant Helium and Iron Abundances
- Volume 7, Issue 24 - article #11
- Don A. VandenBerg, Peter A. Bergbusch, Aaron Dotter, Jason W. Ferguson, Georges Michaud, Jacques Richer, Charles Proffitt
- arXiv.org - Astrophysics - Volume: 2012, Issue: 15 Jun
- arXiv:1206.1820 [pdf, ps, other]
The Victoria-Regina Stellar Models: Evolutionary Tracks and Isochrones for a Wide Range in Mass and Metallicity that Allow for Empirically Constrained Amounts of Convective Core Overshooting
- Volume 1, Issue 4 - article #7
- Don A. VandenBerg, Peter A. Bergbusch, and Patrick D. Dowler
- ABSTRACT, FULL TEXT, PDF (881 kB), PS

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