Radial and nonradial oscillations of partially-degenerate stellar masses

Details Radial and nonradial oscillations of partially-degenerate stellar masses Radial and nonradial oscillations of partially-degenerate stellar masses

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.116....9d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 116, no. 1, Nov. 1985, p. 9-19.

Statistics

Computation

2

Stellar Mass, Stellar Models, Stellar Oscillations, Computational Astrophysics, Main Sequence Stars, Vibration Mode, White Dwarf Stars

Scientific paper

The radial and nonradial modes of oscillation of partially degenerate stellar masses have been studied. It is found that the radial mode shows a decrease with increased central condensation and the configuration tends, therefore, towards a marginally stable point with increased degeneracy. The nonradial modes for l = 2 and 3 also shows a similar trend. However, the decrease is slower than the corresponding radial mode.

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