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

D. Russeil (1) , M. Pestalozzi , J. C. Mottram , Sylvain Bontemps (2, 3, 4, 5) , L. D. Anderson (1) , Annie Zavagno (1, 6) , M. T. Beltran , J. Bally , J. Brand , C. Brunt , R. Cesaroni (7) , G. Joncas , D. Marshall (8) , P. Martin , F. Massi (9) , S. Molinari (10) , T. Moore , A. Noriega-Crespo , L. Olmi (11) , M. A. Thompson , M. Wienen (12) , F. Wyrowski (12)

1 LAM - Laboratoire d'Astrophysique de Marseille
2 OASU - Observatoire aquitain des sciences de l'univers
3 UB - Université Sciences et Technologies - Bordeaux 1
4 LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
5 L3AB - Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux
6 OAMP - Observatoire Astronomique de Marseille Provence
7 OAA - INAF - Osservatorio Astrofisico di Arcetri
8 CESR - Centre d'étude spatiale des rayonnements
9 LaMCoS - Laboratoire de Mécanique des Contacts et des Structures [Villeurbanne]
10 IFSI - Istituto di Fisica dello Spazio Interplanetario
11 ARENA - Antarctic Research a European Network for Astrophysics
12 MPIFR - Max-Planck-Institut für Radioastronomie

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 $^{13}$CO 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 $^{13}$CO and C$^{18}$O J=1-0 observations obtained as part of the Exeter-FCRAO CO Galactic Plane Survey (Brunt et al., in prep.). (2 data files).

Mots clés: Galactic plane; H II regions; Stars: distances; Spectroscopy

Domaines: Astrophysique stellaire et solaire [astro-ph.SR]

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⟩