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Warm neutral halos around molecular clouds. II - H I and CO (J = 1-0) observationsObservational data are presented relating to the boundary regions between dense, molecular clouds and the more diffuse atomic gas. The data set consists of H I 21 cm and CO (J = 1-0) strip maps in 14 molecular clouds which traverse 62 known CO cloud boundaries. The angular lengths of the strips range from 0.5 deg to several degrees of arc, which is generally adequate to eliminate confusion with background (and foreground) H I. Most of the crossed boundaries (49 of 62) show clear evidence for the presence of H I emission maxima, or halos, lying outside the molecular clouds' gas. There is also general evidence for limb brightening in the CO emission.
Document ID
19910045705
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Wannier, Peter G.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lichten, Steven M.
(JPL Pasadena, CA, United States)
Andersson, B.-G.
(JPL, Pasadena; California, University Los Angeles; Goteborg, University, Sweden)
Morris, Mark
(California, University Los Angeles, United States)
Date Acquired
August 14, 2013
Publication Date
April 1, 1991
Publication Information
Publication: Astrophysical Journal Supplement Series
Volume: 75
ISSN: 0067-0049
Subject Category
Astrophysics
Accession Number
91A30328
Funding Number(s)
CONTRACT_GRANT: NSF AST-87-18068
Distribution Limits
Public
Copyright
Other

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