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Massive Star Forming Regions in the Galactic Plane: A Comparative Study Using BGPS, Spitzer, & Optical/Near-IR Surveys

Published online by Cambridge University Press:  21 October 2010

Guy S. Stringfellow
Guy S. Stringfellow
Affiliation:
CASA, University of Colorado, 389 UCB, Boulder, CO, USA, Guy.Stringfellow@colorado.edu
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Abstract

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The Bolocam Galactic Plane Survey (BGPS) is a 1.1 mm continuum survey that has detected more than 8300 clumps over a 170 square degree survey area in the Galactic plane. The full power of these data is realised only when considering the full complement of data spanning millimetre through x-ray wavelengths.

Keywords

Galaxy: structureISM: jets and outflowsISM: structurestars: formationsurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 805
Copyright
Copyright © International Astronomical Union 2010

References

Aguirre, J. et al. 2009, ApJ Suppl in pressGoogle Scholar
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