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The temperature of large dust grains in molecular cloudsThe temperature of the large dust grains is calculated from three molecular clouds ranging in visual extinction from 2.5 to 8 mag, by comparing maps of either extinction derived from star counts or gas column density derived from molecular observations to I(100). Both techniques show the dust temperature declining into clouds. The two techniques do not agree in absolute scale.
Document ID
19910048943
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/169924
Authors
Clark, F. O. (USAF, Geophysics Laboratory, Hanscom AFB MA, United States)
Laureijs, R. J. (JPL Pasadena, CA, United States)
Prusti, T. (Laboratory for Space Research Groningen, Netherlands)
Date Acquired
August 14, 2013
Publication Date
April 20, 1991
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 371
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A33566
Funding Number(s)
CONTRACT_GRANT: NATO-0093/88
Distribution Limits
Public
Copyright
Other

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