Published October 1, 1975 | Version v1
Journal article Metadata-only

Microwave H2O emission from young stars

Creators

  • 1. Naval Research Lab., Washington, DC

Description

H2O emission has been detected from the Ae or Be stars HD 250550, LkHα 234, and LkHα 198. Comparison of the H2O velocity with that of associated interstellar CO indicates that the H2O originates in an infall region, possibly the contracting parent cloud. H2O emission has also been detected in OH 205.1--14.1, and OH source near the T Tauri star LkHα 308

Additional details

Identifiers

DOI
10.1086/181933;

Publishing Information

Journal Title
The Astrophysical Journal
Journal Volume
201
Journal Issue
1
Series
Astrophys. J., Lett.
Journal Page Range
L27
ISSN
0004-637X

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
7247120
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
CARBON MONOXIDE; INTERSTELLAR SPACE; MICROWAVE RADIATION; MOLECULES; NEBULAE; STARS; WATER
Descriptors DEC
CARBON COMPOUNDS; CARBON OXIDES; CHALCOGENIDES; ELECTROMAGNETIC RADIATION; HYDROGEN COMPOUNDS; OXIDES; OXYGEN COMPOUNDS; RADIATIONS; SPACE

Optional Information

Notes
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