A new helium variable.
Abstract
The B-type star HD 175362 has been found to be a spectrum variable with a period of 3.7 days. The strongest variation occurs for the helium lines, but silicon and other lines are also suspected to vary, both in strength and width.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- February 1974
- DOI:
- 10.1093/mnras/166.1.35P
- Bibcode:
- 1974MNRAS.166P..35B