Physics
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3603d&link_type=abstract
ATNF proposal M570, Semester: October, 2010
Physics
Star Formation, Interstellar Medium In And Around The Milky Way, Mopra
Scientific paper
HESS J1626-490 is one of a growing number of unidentified TeV gamma-ray sources without an obvious classical high-energy counterpart such as a supernova remnant, a pulsar-powered nebula or X-ray binary. CO(1-0), HI and 12mm survey (HOPS) observations reveal interesting overlapping molecular and atomic gas features which may be related to high mass star formation and possibly a nearby supernova remnant SNR G335.2+0.1. This project will investigate in much more detail the dense gas towards the molecular gas, TeV emission and SNR. We will use the CS(1-0) SiO(1-0) and NH3 transitions to probe for shocks and/or disruption that will give further clues as to the physical association of the molecular gas and high-mass star formation processes to the gamma-ray emission.
Aharonian Felix
Burton Michael
Dawson Bruce
de Wilt Phoebe
Eger Peter
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