Submillimetre Imaging of Candidate High-Mass Protostellar Objects

Details Submillimetre Imaging of Candidate High-Mass Protostellar Objects Submillimetre Imaging of Candidate High-Mass Protostellar Objects

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..369f&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

A sample of IRAS selected, radio quiet, sources with colours similar to ultracompact (UC) HII regions have been imaged at mid-infrared and submillimetre wavelengths. The submillimetre emission imaged with SCUBA shows the sources to have a range of morphologies and modelling indicates that the circumstellar envelopes of these sources have flatter density profiles than UC HII regions.

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