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A rotational-state population analysis of the high-resolution IUE observation of CS emission in comet P/HalleyThe high resolution spectrum of comet P/Halley has been measured in the region of the CS emission. CS in comet Halley is produced by photodissociation of CS2 and subsequently reexcited by broad band solar radiation. An inversion procedure is introduced to extract the rotational population distribution from the dispersed fluorescence spectrum. Intensity anomalies in the wavelength region corresponding to P and Q branch emission are considered.
Document ID
19880036231
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Prisant, M. G. (California, University Berkeley, United States)
Jackson, W. M. (California, University Davis, United States)
Date Acquired
August 13, 2013
Publication Date
November 1, 1987
Publication Information
Publication: Astronomy and Astrophysics
Volume: 187
Issue: 1-2
ISSN: 0004-6361
Subject Category
Astrophysics
Accession Number
88A23458
Funding Number(s)
CONTRACT_GRANT: NAGW-903
CONTRACT_GRANT: NAGW-446
Distribution Limits
Public
Copyright
Other

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