CO(J=2->1) In-Plane Survey of the 4th Galactic Quadrant.

Details CO(J=2->1) In-Plane Survey of the 4th Galactic Quadrant. CO(J=2->1) In-Plane Survey of the 4th Galactic Quadrant.

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001rmxac..11...67l&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We present CO(J=2 -> 1) data covering from 270o to 360o in Galactic longitude, at latitude b=0o (IV quadrant). These data were obtained with the VST2 (Very Small Telescope 2), a 60 cm antenna with a beam of 8.9 arcmin (FWHM) installed by the University of Tokyo at ESO La Silla, Chil e (Hasegawa et al. 1996). The new data are analyzed under a similar axisymmmetric model from Sakamoto et al. (1997) for b=0o, and using published CO(J=1 -> 0) data by Bronfman et al. (1989). The distribution of the TR*({J=2 -> 1})/TR*({J=1 -> 0}) ratio is compared to that of massive star forming regions from the catalogs of Bronfman et al. (1996) and Caswell & Haynes (1987).

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