The asynchronously rotating Algol binaries U Sagittae and RY Persei

Details The asynchronously rotating Algol binaries U Sagittae and RY Persei The asynchronously rotating Algol binaries U Sagittae and RY Persei

Nov 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aj.....92.1168v&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 92, Nov. 1986, p. 1168-1177.

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30

Astronomical Photometry, Binary Stars, Stellar Rotation, Angular Velocity, Astronomical Spectroscopy, Light Curve, Stellar Mass

Scientific paper

A statistical base is developed from rotation rates and other parameters of two Algol-type binaries, in order to deepen understanding of rapid rotation in Algol primary stars and possible evolutionary links to the W Serpetis systems. A process is presented by means of which self-consistent solutions that fit the data can be obtained, in cases where the wavelength dependences of computed stellar atmosphere fluxes disagree with those of the observed binary.

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