Chandrasekhar's perturbation method-oriented theories up to third order - Structure parameters for rotating polytropic stars

Details Chandrasekhar's perturbation method-oriented theories up to third order - Structure parameters for rotating polytropic stars Chandrasekhar's perturbation method-oriented theories up to third order - Structure parameters for rotating polytropic stars

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apjs...66..139g&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 66, Feb. 1988, p. 139-149.

Statistics

Computation

6

Computational Astrophysics, Perturbation Theory, Stellar Interiors, Stellar Rotation

Scientific paper

In this paper we present numerical results for the structure parameters
of an either uniformly or differentially rotating polytropic star. In
the computations we employ a Chandrasekhar's method-oriented
perturbation theory up to third order.

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