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The Z-dependence of the Spin Temperature of HIResults relating to the following aspects of hydrogen clouds are presented: (1) the vertical distribution of cold H T clouds; (2) possible systematic warming of H T clouds at high absolute values of z; (3) possible increase of the fraction of warm intercloud medium H T with high absolute values of z; and (4) the effect of optical depth on previous H T emission surveys.
Document ID
19850007271
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Kulkarni, S. R. (California Univ. Berkeley, CA, United States)
Heiles, C. (California Univ. Berkeley, CA, United States)
Vangorkom, J. (National Radio Astronomy Observatory Socorro, N. Mex., United States)
Dickey, J. M. (Minnesota Univ. Minneapolis, United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1984
Publication Information
Publication: NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81
Subject Category
Astrophysics
Accession Number
85N15580
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19850007230Collected WorksLocal Interstellar Medium. International Astronomical Union Colloquium No. 81
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