``Anti-humps" in the dwarf nova RZ Leonis
Abstract
We report the discovery of broad absorption features in the light curve of RZ Leo developing into normal emission humps in a period of two months. This secular change is accompanied by an increase of the systemic luminosity by about 45.
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- February 1999
- Bibcode:
- 1999IBVS.4672....1M
- Keywords:
-
- cataclysmic variables;
- dwarf novae;
- accretion disks