Department of Physics and Astronomy: Publications and Other Research
Date of this Version
1995
Document Type
Article
Citation
Astrophysical Applications of Powerful New Databases, ASP Conference Series, Vol. 78,1995.
Abstract
We describe modeling of the ''beat'' and "bump" Cepheids, using the new radiative opacities. Discrepancies between these models and the evolutionary tracks for stars of appropriate mass are discussed. Finally, we point out some of the difficulties involving the long-period Cepheid sample with periods greater than 20 days.
COinS
Comments
Copyright 1995 Astronomical Society of the Pacific