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Evolution of the ultraviolet coma of comet Austin (1982g.)Ultraviolet spectra of comet Austin (1982) obtained in July 1982 at heliocentric distances ranging from 1.10 to 0.81 AU preperihelion with the IUE reveal that the comet is very similar in chemical composition and appearance to comet Bradfield (1979X). In addition, the derived H2O production rate is found to vary with heliocentric distance as r to the -3.6, similar to the r to the -3.7 behavior found for comet Bradfield. It is pointed out, however, that the limited sample rate precludes the observation of the short-term variations which could be produced by a rotating nonuniform cometary nucleus.
Document ID
19840049422
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Feldman, P. D.
(Johns Hopkins University Baltimore, MD, United States)
Ahearn, M. F.
(Johns Hopkins Univ. Baltimore, MD, United States)
Schleicher, D. G.
(Maryland, University College Park, MD, United States)
Festou, M. C.
(CNRS, Service d'Aeronomie, Verrieres-le-Buisson Essonne, France)
Wallis, M. K.
(University College Cardiff, United Kingdom)
Burton, W. M.
(Science and Engineering Research Council, Rutherford Appleton Laboratory, Didcot Oxon, United Kingdom)
Hughes, D. W.
(Sheffield, University Sheffield, United Kingdom)
Keller, H. U.
(Max-Planck-Institut fuer Aeronomie Katlenburg, Germany)
Benvenuti, P.
(ESA Madrid, Spain)
Date Acquired
August 12, 2013
Publication Date
February 1, 1984
Publication Information
Publication: Astronomy and Astrophysics
Volume: 131
Issue: 2 Fe
ISSN: 0004-6361
Subject Category
Astrophysics
Accession Number
84A32209
Funding Number(s)
CONTRACT_GRANT: NSG-5393
CONTRACT_GRANT: NAG5-279
Distribution Limits
Public
Copyright
Other

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