Light curve Variations in Short-Period Eb-Type Contact Binaries

Details Light curve Variations in Short-Period Eb-Type Contact Binaries Light curve Variations in Short-Period Eb-Type Contact Binaries

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984msngr..35...38m&link_type=abstract

The Messenger, No. 35, P.38, 1984

Physics

4

Scientific paper

The structure and evolution of contact binaries is still very poorly understood. If two stars are so close together that they are physically touching, then it is to be expected that the normal equilibrium configurations of the single stars are heavily disturbed. Mass and energy transfer between the components can occur which makes the theoretical calculations on stellar structure and evolution extremely difficult.

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