Hi-Gal sources distance determination (Russeil+, 2011)

Details Hi-Gal sources distance determination (Russeil+, 2011) Hi-Gal sources distance determination (Russeil+, 2011)

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..35269151r&link_type=abstract

VizieR On-line Data Catalog: J/A+A/526/A151. Originally published in: 2011A&A...526A.151R

Physics

Galactic Plane, H Ii Regions, Stars: Distances, Spectroscopy

Scientific paper

We obtain velocities along the line of sight to Hi-GAL sources, where possible, using CO data observed with the SEQUOIA receiver on the FCRAO 14m telescope. In the l=30 ° region we use the 13CO J=1-0 data from the BU-FCRAO Galactic Ring Survey (GRS, Jackson et al., 2006ApJS..163..145J) while in the l=59° region we use 13CO and C18O J=1-0 observations obtained as part of the Exeter-FCRAO CO Galactic Plane Survey (Brunt et al., in prep.).
(2 data files).

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