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Evolutionary sequences for Nova V1974 Cygni using new nuclear reaction rates and opacities
Authors:S. Starrfield,J. W. Truran,M. C. Wiescher,&   W. M. Sparks
Affiliation:Department of Physics and Astronomy, Arizona State University, PO Box 871504, Tempe, AZ 85287-1504, USA,;Department of Astronomy and Astrophysics and Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA,;Department of Physics, University of Notre Dame, Notre Dame, IN 46556, USA,;XNH, Nuclear and Hydrodynamic Applications, MS F664, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
Abstract:
Keywords:convection    nuclear reactions    nucleosynthesis    abundances    stars: activity    stars: individual: Nova V1974 Cygni    novae    cataclysmic variables    white dwarfs
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