A detailed line survey of G327.3-0.6

Details A detailed line survey of G327.3-0.6 A detailed line survey of G327.3-0.6

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atnf.prop.1358w&link_type=abstract

ATNF proposal M294, Semester: April, 2008

Physics

Galactic, Mopra

Scientific paper

In 2006, we used the new MOPS on Mopra to survey a large number of high-mass star forming regions. One of the sources surveyed (G327.3-0.6) showed a great wealth of spectral lines, rivalled only by Orion and SGR B2. We detected nearly 600 lines in the 3mm spectrum, with as little as 10 minutes total integration time (5 minutes on source). We wish to study this object in more detail this semester by performing deep integrations of an hour across the 3, 7 and 12mm bands. this will allow us to detect many lines from many species such that we can investigate the detailed chemistry of the source.

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