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Satellites to Lyman-alpha due to protons.Using accurate H2(+) wave functions, the line broadening of the Lyman-alpha wings is calculated. Of particular interest are the linelike satellites which appear prominently at 1233.5, 1240.5, and 1404.9 A. No broadening of Lyman-alpha transition due to protons occurs at wavelengths below 965 A and above 1405 A.
Document ID
19730036090
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/151935
Authors
Stewart, J. C.
Peek, J. M. (Sandia Laboratories Albuquerque, N. Mex., United States)
Cooper, J. (Joint Institute for Laboratory Astrophysics Boulder, Colo., United States)
Date Acquired
August 7, 2013
Publication Date
February 1, 1973
Publication Information
Publication: Astrophysical Journal
Volume: 179
Subject Category
Space Radiation
Accession Number
73A20892
Funding Number(s)
CONTRACT_GRANT: NGR-06-003-057
Distribution Limits
Public
Copyright
Other

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