Two New Eclipsing Binaries: V1626 Ori (Brh V38) and GSC 0486-4828 (Brh V64)
Abstract
V1626 Ori is an EA with a period of 1.137793 days containing a mid F-type main-sequence primary and an oversized early K-type secondary, which may or may not fill its Roche lobe. GSC 0486-4828 has a period of 9.27850 days and contains two apparently unevolved main-sequence stars of spectral types late B and early A.
- Publication:
-
Information Bulletin on Variable Stars
- Pub Date:
- November 2002
- Bibcode:
- 2002IBVS.5339....1L
- Keywords:
-
- Eclipsing binaries;
- variable stars;
- photometry