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

Abstract : 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 C18^O 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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Contributor : Marie-Paule Pomies <>
Submitted on : Wednesday, September 7, 2011 - 1:41:05 PM
Last modification on : Monday, November 23, 2020 - 2:44:07 PM



D. Russeil, M. Pestalozzi, J. C. Mottram, Sylvain Bontemps, L. D. Anderson, et al.. Hi-Gal sources distance determination (Russeil+, 2011). 2011, pp.69151. ⟨hal-00620157⟩



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