Identifying molecular clouds associated with TeV-emitting SNR G347.3-0.5

Details Identifying molecular clouds associated with TeV-emitting SNR G347.3-0.5 Identifying molecular clouds associated with TeV-emitting SNR G347.3-0.5

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atnf.prop.2676l&link_type=abstract

ATNF proposal M137, Semester: October, 2009

Physics

Mopra

Scientific paper

We propose to map selected regions towards the supernova remnant G347.3-0.5 in order to test claims of associations with different molecular clouds. This SNR is suggested to be the first unambiguous accelerator of Galactic cosmic ray nuclei, although the nature of the TeV emission from the SNR is still uncertain. Our observations will use optically thin 13CO transition and will have higher spatial resolution than previous observations, which could confirm or reject the suggested associations. These results will provide important constraints for the broad-band model of particle acceleration in this remnant.

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