Star-forming complexes in the Galaxy (Russeil+, 2003)

Details Star-forming complexes in the Galaxy (Russeil+, 2003) Star-forming complexes in the Galaxy (Russeil+, 2003)

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33970133r&link_type=abstract

VizieR On-line Data Catalog: J/A+A/397/133. Originally published in: 2003A&A...397..133R

Computer Science

H Ii Regions, Stars: Distances, Radial Velocities

Scientific paper

We have carried out a multiwavelength study of the plane of our Galaxy in order to establish a star-forming-complex catalogue which is as complete as possible. Features observed include Hα, H109α, CO, the radio continuum and absorption lines. For each complex we have determined the position, the systemic velocity, the kinematic distance and, when possible, the stellar distance and the corresponding uncertainties. All of these parameters were determined as homogeneously as possible, in particular all the stellar distances have been (re)calculated with the same calibration and the kinematic distances with the same mean Galactic rotation curve. Through the complexes with stellar distance determination, a rotation curve has been fitted. It is in good agreement with the one of Brand & Blitz (1993, Cat. ).
(2 data files).

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