Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995cait.rept.....p&link_type=abstract
Final Report, 1 Aug. 1994 - 31 Jul. 1995 California Inst. of Tech., Pasadena, CA.
Astronomy and Astrophysics
Astronomy
Angular Resolution, H Ii Regions, Infrared Astronomy, Infrared Radiation, Interplanetary Dust, Massive Stars, Star Formation, Submillimeter Waves, Emission Spectra, Interstellar Matter, Luminosity, Molecular Clouds, Stellar Evolution
Scientific paper
The primary objective of the research funded under this grant has been to perform a high angular resolution mapping survey of the far-infrared and submillimeter continuum emission from the dust cocoons surrounding young, deeply embedded massive stars and the ultracompact H II regions they create. The high infrared, submillimeter, and radio luminosity makes the ultracompact H II regions ideal tracers of current high-mass star formation. Detailed investigations of their structure, evolution, and interaction with their parent molecular clouds are thus important for understanding the early evolutionary phases of massive main sequence stars, the nature of the dense molecular cores in which they form, and the relationship to coeval low-mass star formation.
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