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P/Halley: Spatial distribution and scale lengths for C2, CN, NH2, and H2OFrom P/Halley, long slit spectroscopic exposures on 12 dates, extending from Oct. 1985 to May 1986, spatial profiles were obtained for emissions by C2, CN, NH2, and OI ((sup 1)D). Examples of our derived spatial profiles are given. The qualitative trend of the scale lengths for the different species is nicely exemplified in this example. C2 has the longest parent scale length followed by CN and NH2. OI which tracks the parent H2O distribution is quite narrow but slightly wider than the continuum profile which has a center essentially indistinguishable from the stellar seeing disk. Comparison of C2 and CN also shows that C2 is falling off faster in the wings so that the daughter scale length of CN must be larger than that of C2.
Document ID
19930009968
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Fink, Uwe
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Combi, Michael
(Michigan Univ. Ann Arbor., United States)
Disanti, Michael A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991
Subject Category
Astrophysics
Accession Number
93N19157
Funding Number(s)
CONTRACT_GRANT: NAGW-1549
CONTRACT_GRANT: NAGW-1907
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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