Published April 1, 1976 | Version v1
Journal article Metadata-only

OH-IR stars. I. Physical properties of circumstellar envelopes

Creators

  • 1. California Institute of Technology

Description

The predicted values of the gas temperature, T, and the OH abundance, n/subO//subH/, depend upon the rate of mass loss from the central star, Phi. The results quoted above are based on a calculation with Phi=3 x 10-5 M/sub sun/ yr-1. In general, T varies inversely and n/sub OH/ varies directly with Phi

Additional details

Identifiers

DOI
10.1086/154257;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
205
Journal Issue
1
Series
Astrophys. J.
Journal Page Range
144
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
7274268
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CHEMICAL REACTIONS; COLLISIONS; COSMIC DUST; COSMIC GASES; COSMOCHEMISTRY; HYDROXYL RADICALS; INFRARED RADIATION; INTERSTELLAR GRAINS; PHYSICAL PROPERTIES; STELLAR ATMOSPHERES; WATER
Descriptors DEC
ATMOSPHERES; CHEMISTRY; DUSTS; ELECTROMAGNETIC RADIATION; FLUIDS; GASES; HYDROGEN COMPOUNDS; OXYGEN COMPOUNDS; PARTICLES; RADIATIONS; RADICALS

Optional Information

Notes
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