A search for OH 6049 MHz emission towards supernova remnants

Details A search for OH 6049 MHz emission towards supernova remnants A search for OH 6049 MHz emission towards supernova remnants

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atnf.prop..389w&link_type=abstract

ATNF proposal P495, Semester: April, 2006

Computer Science

Galactic, Parkes

Scientific paper

The 6049 MHz transition within the first excited rotational state of OH is the analogue of the 1720 MHz transition in the ground rotational state. It is inverted by collisions under similar densities and temperatures, but requires larger OH column densities to give significant amplification. It is potentially a complementary indicator of supernova remnant - molecular cloud interactions. We propose to search for emission in this transition from supernova remnants that show evidence of cloud interactions.

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