The orbital period changes of UX Ursae Majoris

Details The orbital period changes of UX Ursae Majoris The orbital period changes of UX Ursae Majoris

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103.1258r&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Dec. 1991, p. 1258-1263.

Astronomy and Astrophysics

Astronomy

20

Accretion Disks, Cataclysmic Variables, Eclipsing Binary Stars, Main Sequence Stars, Stellar Orbits, White Dwarf Stars, Stellar Rotation, Stellar Spectrophotometry

Scientific paper

It is found that the orbital changes of the eclipsing cataclysmic variable UX Ursae Majoris are aperiodic. This eliminates apsidal motion and the revolution of the eclipsing system around a third body as feasible explanations of the period variations. An origin in the magnetism of the secondary appears possible, but the details are not clear.

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