Tag Archives: H-R

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

Don A. VandenBerg (1), Peter A. Bergbusch (2), Aaron Dotter (3), Jason W. Ferguson (4), Georges Michaud (5), Jacques Richer (6) & Charles R. Proffitt (7) ((1) Department of Physics & Astronomy, University of Victoria, P.O. Box 3055, Victoria, B.C., … Continue reading

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