The structure of BB Doradus in quiescence
Abstract
Spectroscopic observations during a low state of BB Dor reveal a complex emission distribution. Irradiation by the white dwarf as well as magnetic fields of the secondary star are needed for an explanation.
- Publication:
-
Revista Mexicana de Astronomia y Astrofisica Conference Series
- Pub Date:
- October 2011
- Bibcode:
- 2011RMxAC..40..288S
- Keywords:
-
- accretion;
- accretion disks;
- stars: activity;
- stars: magnetic field;
- stars: variables: general