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

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

Nov 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010hia....15..805s&link_type=abstract

Highlights of Astronomy, Volume 15, p. 805-805

Astronomy and Astrophysics

Astronomy

Galaxy: Structure, Ism: Jets And Outflows, Ism: Structure, Stars: Formation, Surveys

Scientific paper

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.

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