CO survey of galactic molecular clouds. II. (Bieging+, 2011)

Details CO survey of galactic molecular clouds. II. (Bieging+, 2011) CO survey of galactic molecular clouds. II. (Bieging+, 2011)

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..21960018b&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/196/18. Originally published in: 2011ApJS..196...18B

Physics

Molecular Clouds, Radio Lines, H Ii Regions, Interstellar Medium, Millimetric/Submm Sources

Scientific paper

Observations were made with the Heinrich Hertz Submillimeter Telescope (HHT) on Mt. Graham, AZ; in several observing sessions from 2005 June to 2008 April. The J=2-1 lines of the CO isotopologues 12C16O (hereafter CO) and 13C16O (hereafter 13CO) were mapped over a 2.00°x1.67° field covering the galactic coordinate ranges l=132.5° to 134.5°, b=0° to +1.67°.
(1 data file).

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