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Title:
Shocked molecular material associated with the supernova remnant G33.6 + 0.1?
Authors:
Green, D. A.; Dewdney, P. E.
Affiliation:
AA(Mullard Radio Astronomy Observatory, Cambridge, England), AB(Dominion Radio Astrophysical Observatory, Penticton, Canada)
Publication:
Royal Astronomical Society, Monthly Notices (ISSN 0035-8711), vol. 254, Feb. 15, 1992, p. 686-692. (MNRAS Homepage)
Publication Date:
02/1992
Category:
Astrophysics
Origin:
STI
NASA/STI Keywords:
INTERSTELLAR MATTER, MOLECULAR CLOUDS, SHOCK WAVES, SUPERNOVA REMNANTS, ABSORPTION SPECTRA, CARBON MONOXIDE, FORMYL IONS, H I REGIONS
Bibliographic Code:
1992MNRAS.254..686G

Abstract

Results of (C-12)O J = 1 - 0 and HCO(+) J = 1 - 0 observations towards the supernova remnant G33.6 + 0.1 made with the NRAO 12-m telescope are presented. Strong CO emission was observed toward G33.6 + 0.1, with components over a wide range of velocities. Bright extended HCO(+) emission was detected at velocities near + 105 km/s, in the area of the eastern portion of the remnant, where there is corresponding CO emission from the adjacent molecular cloud at the same velocities. There are also several compact H II regions associated with the molecular cloud. The results provide a direct indication of interaction of this remnant with the adjacent molecular cloud.

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