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Interstellar photoelectric absorption cross sections, 0.03-10 keVAn effective absorption cross section per hydrogen atom has been calculated as a function of energy in the 0.03-10 keV range using the most recent atomic cross section and cosmic abundance data. Coefficients of a piecewise polynomial fit to the numerical results are given to allow convenient application in automated calculations.
Document ID
19830056692
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/161102
Authors
Morrison, R. (Wisconsin Univ. Madison, WI, United States)
Mccammon, D. (Wisconsin, University Madison, WI, United States)
Date Acquired
August 11, 2013
Publication Date
July 1, 1983
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 270
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
83A37910
Funding Number(s)
CONTRACT_GRANT: NGL-50-002-044
Distribution Limits
Public
Copyright
Other

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