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Radar interferometric studies of cometsOur objectives are to use radio interferometry to study composition, velocity distribution, maser excitation, and plasma interactions of cometary gas. Two new cometary chemistry programs were started with radio interferometers: (1) the VLA used to search for HC3N emission from Comet Brorsen-Metcalf at 3.3 cm wavelength; and (2) the BIMA millimeter array used to observe Comet Austin in HCN.
Document ID
19920003627
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Snyder, Lewis E.
(Illinois Univ. Chicago., United States)
Palmer, Patrick
(Chicago Univ. IL., United States)
Depater, Imke
(California Univ. Berkeley., United States)
Date Acquired
September 6, 2013
Publication Date
October 1, 1991
Publication Information
Publication: NASA, Washington, Reports of Planetary Astronomy, 1991
Subject Category
Astronomy
Accession Number
92N12845
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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