BG CMi time keeping
Abstract
Twelve seasons, from 2005 to 2016, of photometric monitoring of the intermediate polar BG CMi are presented and are compared with previous observations. The spin up of the white dwarf is found to have undergone a major change between 1996 and 2005. There is also some evidence for sideband signals.
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- May 2016
- DOI:
- 10.48550/arXiv.2011.04982
- arXiv:
- arXiv:2011.04982
- Bibcode:
- 2016IBVS.6168....1B
- Keywords:
-
- photometry;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- IBVS 6168 (2016)