Carbon Abundance in Early B-Stars. I. NLTE Calculations for ΓPeg.
Abstract
NLTE calculations of carbon abundance in γPeg atmosphere revealed a slight deficiency of this element ([C/H] =‑0.25). A short discussion of this result is given. The list of CII that could be used for LTE calculation of carbon abundance in hot stars is presented.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- December 1998
- DOI:
- Bibcode:
- 1998Ap&SS.260..531K
- Keywords:
-
- Atmosphere;
- Short Discussion;
- Carbon Abundance;
- Slight Deficiency;
- NLTE Calculation