Emission-line flare of ES 560B
Abstract
Strong Balmer emission lines are found in the spectrum of ES 560B. It is for the first time during our observations of this star from 1996. The star is a fainter component of the visual double system, its V 10.5 .
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- April 2002
- Bibcode:
- 2002IBVS.5261....1S
- Keywords:
-
- spectroscopy