Wolf-Rayet stars. V. The temperature stratification.
Abstract
The behavior of C iii AS 696 with changing spectral subclass is interpreted in terms of the expanding-envelope model to indicate that in the WC stars the temperature must decrease with radius over the bulk of the envelope. Subject headings: atmospheres, stellar - line formation - Wolf-Rayet stars
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 1973
- DOI:
- 10.1086/152005
- Bibcode:
- 1973ApJ...180..783K