Shocked molecular material associated with the supernova remnant G33.6 + 0.1?

Details Shocked molecular material associated with the supernova remnant G33.6 + 0.1? Shocked molecular material associated with the supernova remnant G33.6 + 0.1?

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.254..686g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 254, Feb. 15, 1992, p. 686-692.

Astronomy and Astrophysics

Astronomy

25

Interstellar Matter, Molecular Clouds, Shock Waves, Supernova Remnants, Absorption Spectra, Carbon Monoxide, Formyl Ions, H I Regions

Scientific paper

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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