A simple model of CQ UMa
Abstract
An attempt is made to explain light variations in the blue region of the magnetic star CQ UMa by means of a simple oblique rotator model with one extensive circular dark spot centred to the south magnetic pole. This simple model cannot account for the asymmetry of light curves and different shapes of them in various colours.
- Publication:
-
Magnetic Stars
- Pub Date:
- 1988
- Bibcode:
- 1988mast.conf...67M