The Roche coordinates in non-synchronous binaries

Details The Roche coordinates in non-synchronous binaries The Roche coordinates in non-synchronous binaries

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138...61h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 1, Nov. 1987, p. 61-69.

Statistics

Computation

5

Binary Stars, Roche Limit, Stellar Atmospheres, Stellar Rotation, Stellar Spectra, Stellar Winds, Computational Astrophysics, Radiative Heat Transfer, Spherical Coordinates

Scientific paper

The Cayley-Darboux (1872 and 1898) problem for the Roche model of binaries is studied. Roche coordinates are defined as continuations of asymptotically spherical coordinates which are perpendicular to the equipotential layers, but not mutually perpendicular. These coordinates are then obtained in the form of a power series of potential for the general case of nonsynchronous binaries with eccentric orbits.

Affiliated with

Also associated with

No associations

Rating

The Roche coordinates in non-synchronous binaries does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Roche coordinates in non-synchronous binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Roche coordinates in non-synchronous binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1713144