DY Per: Extremely Cool Galactic RCB Star?
Abstract
Observations of the extremely cool RCB candidate, DY Per, are presented to specify its fundamental parameters and evolutionary status. CCD BVRI photometry and spectroscopy was carried out in 2002/2004. A qualitative analysis was made relative to the typical carbon stars of various types.
- Publication:
-
Hydrogen-Deficient Stars
- Pub Date:
- July 2008
- Bibcode:
- 2008ASPC..391...49Z