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OH and CH continuous opacity in solar and stellar atmospheresContinuous absorption cross sections of OH and CH have been computed for the temperature range 1000 K to 9000 K. Both OH and CH produce significant ultraviolet opacity in the sun and cool stars. CH is also significant in the visible at 400 nm.
Document ID
19880031889
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/165794
Authors
Kurucz, Robert L. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Van Dishoeck, Ewine F. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Tarafdar, S. P. (Tata Institute of Fundamental Research Bombay, India)
Date Acquired
August 13, 2013
Publication Date
November 15, 1987
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 322
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
88A19116
Funding Number(s)
CONTRACT_GRANT: NSF PHY-82-17352
CONTRACT_GRANT: NSG-7054
CONTRACT_GRANT: NSF AST-85-18990
Distribution Limits
Public
Copyright
Other

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