Be stars with large magnitude changes.
Abstract
Photoelectric UBV observations of 19 Be stars are listed which in a time interval of eleven years exhibit changes in V larger than AV> . Their light curves display very different shapes; no general rule for the light variation is evident. Key words: variable stars - Be stars - UBV photometry
- Publication:
-
Publications of the Astronomical Society of the Pacific
- Pub Date:
- August 1975
- DOI:
- 10.1086/129818
- Bibcode:
- 1975PASP...87..603F