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A CS survey of massive stars embedded in molecular clouds

Published online by Cambridge University Press:  03 August 2017

L. Bronfman ,
J. May ,
L. A. Nyman  and
P. Thaddeus
L. Bronfman
Affiliation:
Universidad de Chile
J. May
Affiliation:
Universidad de Chile
L. A. Nyman
Affiliation:
Onsala Space Observatory
P. Thaddeus
Affiliation:
Center for Astrophysics

Abstract

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the CS J=2 →1 molecular line at 98 GHz, a normally optically thin line requiring high densities to be excited, has been detected with SEST (Swedish ESO Submillimeter Telescope) toward 294 IRAS pointlike sources having the characteristic FIR colors of embedded stellar objects and apparently associated with the largest molecular cloud complexes in the southern Milky Way. We present here their Galactocentric radial distribution and a correlation between their FIR and CS luminosities.

Information

Type
Large Scale Structure
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 25 - 28
Copyright
Copyright © Kluwer 1991 

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