A search for rotational velocity changes among eclipsing binary stars

Details A search for rotational velocity changes among eclipsing binary stars A search for rotational velocity changes among eclipsing binary stars

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pasp...96..376o&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 96, May 1984, p. 376-381. NSF-supported research.

Astronomy and Astrophysics

Astronomy

44

Angular Velocity, Eclipsing Binary Stars, Stellar Mass Accretion, Stellar Rotation, Hot Stars, Mass Transfer, Spectral Line Width, Stellar Spectra

Scientific paper

The rotations of 26 close binary stars are compared, as they were
observed at three epochs separated by five to twelve years. Significant
changes in the rotation of the hot gainer are noted in three Algol
systems. The implications of these changes for sporadic mass flows known
to occur among Algols are discussed briefly.

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