Slowly-rotating partially-degenerate standard model

Details Slowly-rotating partially-degenerate standard model Slowly-rotating partially-degenerate standard model

Nov 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.116..131d&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 116, no. 1, Nov. 1985, p. 131-139.

Astronomy and Astrophysics

Astrophysics

2

Late Stars, Stellar Models, Stellar Rotation, Stellar Structure, Degeneration, Stellar Evolution, White Dwarf Stars

Scientific paper

The equilibrium structure parameter of slowly rotating, partially degenerate stellar configurations are computed for different values of the central degeneracy parameter. For increased degeneracy at the center, the models are more centrally condensed, and thus the eccentricity of the configuration increases. This results in more severe rotational effects in the outer layers of the configuration.

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