Published March 15, 1974 | Version v1
Journal article Metadata-only

Solid particles and stellar mass loss

Creators

  • 1. Department of Physics and Astronomy, University of Iowa, Iowa City, Iowa 52242

Description

Extensive model atmosphere calculations for cool giants and supergiants show that solid particles do not cause mass loss in such stars. Subject headings: circumstellar shells - late-type stars - mass loss

Additional details

Additional titles

Augmented title (English)
Circumstellar shells, cool giants and supergiants

Identifiers

DOI
10.1086/181441;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
188
Journal Issue
3
Series
Astrophys. J., Lett.
Journal Page Range
L91
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
5147437
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CORRELATIONS; COSMIC DUST; GIANT STARS; INFRARED RADIATION; MASS TRANSFER; OPACITY; STELLAR ATMOSPHERES; SUPERGIANT STARS
Descriptors DEC
ATMOSPHERES; DUSTS; ELECTROMAGNETIC RADIATION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; STARS

Optional Information

Notes
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