Massive Star Formation in MSX Infrared-Dark Clouds

Details Massive Star Formation in MSX Infrared-Dark Clouds Massive Star Formation in MSX Infrared-Dark Clouds

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19913408f&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #134.08; Bulletin of the American Astronomical Society, Vol. 33, p.1503

Astronomy and Astrophysics

Astronomy

Scientific paper

Millimeter and mid-infrared observations have been made of the brightest compact SCUBA 850-micron sources in the MSX infrared-dark clouds (IRDCs) G28.34+0.06, G11.11-0.12, and G79.3+0.3. In two of these sources, Gemini and IRTF observations indicate the presence of nearby massive stars. High-resolution BIMA observations indicate that these stars are interacting with the adjacent molecular gas, possibly triggering the collapse of the compact SCUBA sources.

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