Linear theory radial and nonradial pulsations of DA dwarf stars

Details Linear theory radial and nonradial pulsations of DA dwarf stars Linear theory radial and nonradial pulsations of DA dwarf stars

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pccv.conf...78s&link_type=abstract

Presented at the Conf. on Pulsations in Classical and Cataclysmic Variable Stars, Boulder, Colo., 1-5 Jun. 1982

Computer Science

15

Dwarf Stars, Hydrogen, Stellar Envelopes, Stellar Mass, Carbon, Equations Of State, Gas Mixtures, Helium, Stellar Luminosity, Stellar Models, Stellar Temperature

Scientific paper

The stellar envelope and radial linear nonadiabatic computer code, along with a nonradial code are used to investigate the total hydrogen mass necessary to produce the nonradial instability of DA dwarfs. Opacities and equations of state are obtained for pure mixtures of hydrogen, helium, and carbon. In some cases, a small amount of metals are included in the composition in order to have a variety of mixtures available to make gradual changes in composition from hydrogen to helium. The presence of metals in these mixtures has no effect on the results.

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