The period variations of W Ursae Majoris binaries and their relation to magnetic activity

Details The period variations of W Ursae Majoris binaries and their relation to magnetic activity The period variations of W Ursae Majoris binaries and their relation to magnetic activity

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...250...84v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 250, no. 1, Oct. 1991, p. 84-88.

Astronomy and Astrophysics

Astrophysics

11

Binary Stars, Magnetic Effects, Magnetoactivity, Stellar Evolution, Stellar Magnetic Fields, Late Stars, Main Sequence Stars, Orbital Elements

Scientific paper

The influence of magnetic activity on the period variations of very
close late-type main sequence binaries is studied for W UMa-type contact
systems. In particular, the hypothesis connecting changes of the
inertial and quadrupole moment of the components with period variations
is critically studied and rejected.

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