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OH emission in the direction of TV Gem and BI CygThe NRAO-Green Bank 43-m telescope and 18-cm receiver have detected OH maser main-line emission at 1665 MHz, in the direction of the two late-type supergiants TV Gem and BI Cyg. The detection of the two new OH maser sources is noteworthy in view of the small number of late-type supergiants known to be molecular radio sources, or associated in close proximity with OH emission clouds. The IR, UV and radio properties of the two stars are discussed.
Document ID
19820036103
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/113073
Authors
Brown, L. W. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Hobbs, R. W. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Michalitsianos, A. G. (NASA Goddard Space Flight Center Laboratory for Astronomy and Solar Physics, Greenbelt, MD, United States)
Kafatos, M. (George Mason University Fairfax, VA, United States)
Date Acquired
August 10, 2013
Publication Date
December 1, 1981
Publication Information
Publication: Astronomical Journal
Volume: 86
Subject Category
Astronomy
Accession Number
82A19638
Distribution Limits
Public
Copyright
Other

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