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Tests of shock chemistry in IC 443G

Authors :
Turner, B. E
Chan, Kin-Wing
Green, S
Lubowich, D. A
Source :
Astrophysical Journal, Part 1. 399(1)
Publication Year :
1992
Publisher :
United States: NASA Center for Aerospace Information (CASI), 1992.

Abstract

Eight 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.

Subjects

Subjects :
Astrophysics

Details

Language :
English
ISSN :
0004637X
Volume :
399
Issue :
1
Database :
NASA Technical Reports
Journal :
Astrophysical Journal, Part 1
Notes :
NSF AST-91-00306
Publication Type :
Report
Accession number :
edsnas.19930030007
Document Type :
Report
Full Text :
https://doi.org/10.1086/171908