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Microwave H2O emission from young starsH2O emission has been detected from the Ae or Be stars HD 250550, LkH-alpha 234, and LkH-alpha 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 LkH-alpha 308.
Document ID
19760029638
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/181933
Authors
Schwartz, P. R. (U.S. Navy, E. O. Hulburt Center for Space Research, Washington D.C., United States)
Buhl, D. (NASA Goddard Space Flight Center Astrochemistry Branch, Greenbelt, Md., United States)
Date Acquired
August 8, 2013
Publication Date
October 1, 1975
Publication Information
Publication: Astrophysical Journal
Volume: 201
Subject Category
Astrophysics
Accession Number
76A12604
Distribution Limits
Public
Copyright
Other

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