Physics
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atnf.prop.3655g&link_type=abstract
ATNF proposal C1862, Semester: October, 2010
Physics
Star Formation, Atca
Scientific paper
One of the key problems in the field of star formation is to test if the formation paradigm for low-mass stars, with the presence of an accreting disk and a highly collimated jet, extends to high-mass protostars. We propose to undertake multi-frequency ATCA observations in search for thermal jets towards a sample of ~50 young and luminous massive star forming regions with radio continuum emission much weaker than that expected from their measured IRAS luminosity. These are likely young high-mass objects in the pre-UCHII phase, where the weak radio continuum emission is likely due to the jet phenomena.
Brooks Kate
Garay Guido
Guzman Andres
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