PG 2337+300: a new cataclysmic variable
Abstract
High speed photometry of PG 2337+300 shows flickering on a timescale of minutes. Balmer emission lines are visible in a medium-resolution spectrum. Both these observations indicate that this blue star is a CV.
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- December 1997
- Bibcode:
- 1997IBVS.4539....1K