Detecting Embedded Intermediate-Mass Stars Using Mid-Infrared and H I 21 Centimeter Emission

Details Detecting Embedded Intermediate-Mass Stars Using Mid-Infrared and H I 21 Centimeter Emission Detecting Embedded Intermediate-Mass Stars Using Mid-Infrared and H I 21 Centimeter Emission

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aj....124.3449k&link_type=abstract

The Astronomical Journal, Volume 124, Issue 6, pp. 3449-3464.

Astronomy and Astrophysics

Astronomy

9

Infrared Radiation, Radio Continuum, Radio Emission Lines, Stars: Early-Type, Surveys

Scientific paper

A technique is presented to detect distant, young embedded B stars (and possible clusters) from their imprint on the surrounding interstellar medium. H I 21 cm and 12CO (J=1-0) line data from the Canadian Galactic Plane Survey are combined with mid-infrared images from the Midcourse Space Experiment (MSX) Galactic plane survey to detect the photodissociation regions (PDRs) and molecular gas associated with the embedded intermediate-mass stars. The technique has been applied to a section of the Galaxy covered by the 12CO Five College Radio Astronomy Observatory outer Galaxy survey (102.5d

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