The ellipsoidal variable 33 Tauri. I - Spectroscopic orbit

Details The ellipsoidal variable 33 Tauri. I - Spectroscopic orbit The ellipsoidal variable 33 Tauri. I - Spectroscopic orbit

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86.1394h&link_type=abstract

Astronomical Journal, vol. 86, Sept. 1981, p. 1394-1396. Research supported by the Natural Sciences and Engineering Research Co

Astronomy and Astrophysics

Astronomy

5

Astrometry, Binary Stars, Orbital Elements, Radial Velocity, Stellar Motions, Variable Stars, Circular Orbits, Eccentricity, Ellipsoids

Scientific paper

The orbital elements of the spectroscopic binary 33 Tau, which has recently been recognized to be an ellipsoidal variable, are presented. The first, rough plot of the radial velocities revealed a nearly circular orbit. The approximately zero eccentricity is to be expected in a system in which the components interact so strongly as to produce an ellipsoidal distortion.

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