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Tests of shock chemistry in IC 443GEight molecular species, in the hot dense clump IC 443G, believed to be impacted by the shock wave from the SNR IC 443, are investigated. The clump consists of two distinct regions, one relatively cool, and one hotter and denser. Region 1 contains CO, HCO(+), HCN, and CN, whose abundances may be explained either by ion-molecule chemistry, or by a D shock of 60-90 km/s, passing through a clump of about 100,000/cu cm. Region 2 gives rise to SiO, CS, SO, and H2CO, and requires an ND shock of 5-15 km/s passing through a region of about 1,000,000/cu cm. Observed fractional abundances fit ND shock models if L is about 6.6 x 10 exp 15 cm. In general, observed line widths vary inversely with derived excitation density, while centroid velocities of all species are essentially identical.
Document ID
19930030007
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Turner, B. E.
(National Radio Astronomy Observatory Charlottesville, VA, United States)
Chan, Kin-Wing
(Maryland Univ. College Park, United States)
Green, S.
(NASA Goddard Inst. for Space Studies New York, United States)
Lubowich, D. A.
(Hofstra Univ. Hempstead; American Inst. of Physics, Woodbury, NY, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1992
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 399
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A14004
Funding Number(s)
CONTRACT_GRANT: NSF AST-91-00306
Distribution Limits
Public
Copyright
Other

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