The structure of late-type contact binaries

Details The structure of late-type contact binaries The structure of late-type contact binaries

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...252..137k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 252, no. 1, Dec. 1991, p. 137-154. Research supported by DFG.

Astronomy and Astrophysics

Astrophysics

7

Binary Stars, Late Stars, Stellar Structure, Magnetohydrodynamic Turbulence, Roche Limit, Stellar Motions, Stellar Systems

Scientific paper

A unified treatment of late-type and early-type contact binaries based on the assumption of hydrostatic equilibrium is extended here and applied to late-type systems assuming systems in a steady state with minimized mass motions. A survey of configurations with M/M(solar) = 2 or greater is presented, and the observational facts are shown to agree with the theory.

Affiliated with

Also associated with

No associations

Rating

The structure of late-type contact 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 structure of late-type contact binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The structure of late-type contact binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1536003