The search for protostars using millimeter/submillimeter dust emission as a tracer

Details The search for protostars using millimeter/submillimeter dust emission as a tracer The search for protostars using millimeter/submillimeter dust emission as a tracer

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.212..197m&link_type=abstract

Astrophysics and Space Science, vol. 212, nos. 1-2, p. 197-214

Other

17

Cosmic Dust, Millimeter Waves, Protostars, Star Formation, Submillimeter Waves, Isothermal Processes, Molecular Clouds, Molecular Spectroscopy, Morphology, Ophiuchi Clouds, Reviewing, Searching, Stellar Envelopes, Stellar Models, Tracers

Scientific paper

There are seven main topics considered in the paper: (1) An overview concerning the formation and evolution of protostars; (2) millimeter/submillimeter dust emission--a new tool for investigating high density regions; (3) star formation rates and the number of detectable isothermal protostars; (4) the case of NGC 2024--molecular spectroscopy at its limits; (5) Morphology of low and medium mass star forming clouds--the Ophiuchus Cloud; (6) Morphology of high-mass star forming clouds; and (7) Searching for the low mass protostars.

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