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1990ApJ...362..652S - Astrophys. J., 362, 652-662 (1990/October-2)
A new self-consistent model of circumstellar CO emission for deriving mass-loss rates in red giants. I. The carbon-rich star U Camelopardalis.
SAHAI R.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Infrared: Spectra - Stars: Circumstellar Shells - Stars: Individual Constellation Name: U Camelopardalis - Stars: Late-Type - Stars: Mass Loss
Simbad objects: 13
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