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The spectrum of Comet Austin from 910 to 1180 AA spectrum of Comet Austin (1988 c1) has been obtained from 910 to 1180 A. Three bright emission lines were detected, including a forbidden oxygen line (1128 A), which are attributable to radiative pumping of neutral oxygen by solar Lyman-beta. The relative strengths of the observed features should prove to be a useful diagnostic of the physical conditions and radiation fields in cometary comae. In addition, the absence of strong spectral features from highly volatile species such as He, Ar, or N2 can be used to place constraints on the thermal environment under which the comet was formed and has been processed.
Document ID
19910039976
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Green, James C.
(Colorado Univ. Boulder, CO, United States)
Cash, Webster
(Colorado Univ. Boulder, CO, United States)
Cook, Timothy A.
(Colorado Univ. Boulder, CO, United States)
Stern, S. Alan
(Colorado, University Boulder, United States)
Date Acquired
August 15, 2013
Publication Date
January 25, 1991
Publication Information
Publication: Science
Volume: 251
ISSN: 0036-8075
Subject Category
Astrophysics
Accession Number
91A24599
Funding Number(s)
CONTRACT_GRANT: NSG-5303
Distribution Limits
Public
Copyright
Other

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