The structure of tidally distorted polytropes

Details The structure of tidally distorted polytropes The structure of tidally distorted polytropes

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.100..287s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 100, no. 1-2, March 1984, p. 287-291.

Astronomy and Astrophysics

Astrophysics

1

Cosmology, Perturbation Theory, Polytropic Processes, Rotating Matter, Tides, Mass Ratios, Roche Limit

Scientific paper

The structural parameters of tidally distorted polytropes
(Chandrasekhar, 1933) are calculated numerically, employing the method
developed by Monaghan and Roxburgh (1965) for rotating polytropes. The
results for index (n) values 1.5, 2.0, and 3.0 are presented in tables
and compared to those for the Roche problem.

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