Models of circumstellar molecular radio line emission. Mass loss rates for a sample of bright carbon stars

Astronomy and Astrophysics

Volumn 368, Issue 3, 2001, Pages 969-993

  Schoier F L ^a   Olofsson, H ^a  

^a STOCKHOLM OBSERVATORY   (Sweden)

Author keywords

Circumstellar matter; Radio lines: stars; Stars: AGB and post AGB; Stars: carbon; Stars: late type

Indexed keywords

EID: 0035264387     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010072     Document Type: Article

References (61)