Tracing shocked/disrupted gas towards the TeV gamma-ray supernova remnant CTB 37A

Details Tracing shocked/disrupted gas towards the TeV gamma-ray supernova remnant CTB 37A Tracing shocked/disrupted gas towards the TeV gamma-ray supernova remnant CTB 37A

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3125m&link_type=abstract

ATNF proposal M522, Semester: April, 2010

Mathematics

Logic

Star Formation, Supernovae / Supernovae Remnants, Interstellar Medium In And Around The Milky Way, Mopra

Scientific paper

The gamma-ray-emitting SNR CTB 37A is associated with molecular gas (traced by Nanten2 CO(J=2-1)) and eight 1720.5MHz OH masers, known indicators of gas-shock interactions. We plan to map the gas associated with this SNR at 7mm with Mopra to seek the structure of the shock moving through this region, and dense gas. In these regards, the SiO and CS lines are logical choices.

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