Equi-density surfaces in synchronously rotating close binaries built on polytropic model ν=3

Details Equi-density surfaces in synchronously rotating close binaries built on polytropic model ν=3 Equi-density surfaces in synchronously rotating close binaries built on polytropic model ν=3

Apr 1973

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1973ap%26ss..21..285g&link_type=abstract

Astrophysics and Space Science, Volume 21, Issue 2, pp.285-288

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A direct numerical method, involving no perturbational procedures, is
described and used for the computation of the surfaces of constant
potential, pressure and density in synchronously rotating close binaries
with both components built on polytropic model ν=3.

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