Distances of 793 BGPS sources : J/MNRAS/422/3178

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Authors : Eden D.J. orcid , Moore T.J.T., Plume R. (hide) , Moore T.J.T., Plume R. et..al

VizieR DOI : 10.26093/cds/vizier.74223178
Bibcode : 2012MNRAS.422.3178E (ADS) (Simbad) (Objects)
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CDS Keywords : Molecular clouds; Stars, distances; Radial velocities
UAT : Molecular clouds, Stellar distance, Radial velocity

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Inserted into VizieR : 19-Mar-2013
Last modification : 17-Jul-2024

Star formation towards the Scutum tangent region and the effects of galactic environment. (2012)

Keywords : stars formation - ISM: clouds - ISM: individual objects: W43 - Galaxy: kinematics and dynamics

Abstract:By positional matching to the catalogue of Galactic Ring Survey molecular clouds, we have derived distances to 793 Bolocam Galactic Plane Survey (BGPS) sources out of a possible 806 located within the region defined by Galactic longitudes l=28.5{deg}-31.5{deg} and latitudes |b|<=1{deg}. This section of the Galactic plane contains several major features of Galactic structure at different distances, mainly mid-arm sections of the Perseus and Sagittarius spiral arms and the tangent of the Scutum-Centaurus arm, which is coincident with the end of the Galactic long bar. By utilizing the catalogued cloud distances plus new kinematic distance determinations, we are able to separate the dense BGPS clumps into these three main line-of-sight ...(more)
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Monthly Notices policies

  • J/ApJ/699/1153 : GRS molecular clouds kinematic distances (Roman-Duval+, 2009)
  • J/ApJS/182/131 : Molecular clouds and clumps in the GRS (Rathborne+, 2009)
  • J/ApJ/723/492 : GRS molecular clouds physical properties (Roman-Duval+, 2012)
  • J/ApJ/721/137 : Bolocam Galactic Plane Survey (BGPS) (Bally+, 2010)
  • J/ApJS/188/123 : Bolocam Galactic Plane Survey (BGPS). II. (Rosolowsky+, 2010)
  • J/ApJS/195/14 : Bolocam Galactic Plane Survey (BGPS). V. (Schlingman+, 2011)

                


                

                    

                


                

                    

                


                

                    
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