First results from Mopra HCO+ maps (Barnes+,)

Details First results from Mopra HCO+ maps (Barnes+,) First results from Mopra HCO+ maps (Barnes+,)

Nov 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..21960012b&link_type=abstract

VizieR On-line Data Catalog: J/ApJS/196/12. Originally published in: 2011ApJS..196...12B

Computer Science

Galactic Plane, Molecular Clouds, Interstellar Medium, Velocity Dispersion

Scientific paper

CHaMP began with complete surveys of a large portion of the southern Galactic Plane in four molecular spectral lines in the 3mm waveband made with the 4m Nanten telescope (see Figure 1). A higher-resolution follow-up campaign was then begun to map 209 clumps from the Nanten Master Catalogue (NMC) in a number of 3mm molecular transitions with the 22m diameter Mopra dish of the Australia Telescope National Facility (ATNF) over the period 2004-2007, at much higher sensitivity and angular resolution than with Nanten.
(3 data files).

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