VLA NH3 observations of 5 IRAS sources (Wang+, 2007)

Details VLA NH3 observations of 5 IRAS sources (Wang+, 2007) VLA NH3 observations of 5 IRAS sources (Wang+, 2007)

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34610197w&link_type=abstract

VizieR On-line Data Catalog: J/A+A/461/197. Originally published in: 2007A&A...461..197W

Physics

Infrared Sources, Molecular Clouds, Radio Lines

Scientific paper

The high angular resolution images with the Very Large Array (VLA) allow us to explore the general properties of protostellar cores in massive star forming regions at large distances. We observed the NH3 (J, K)=(1, 1) and (2, 2) lines toward five massive protostar candidates (IRAS 18196-1331, IRAS 18352-0148, IRAS 18361-0627, IRAS 18414-0339 and IRAS 19474+2637) with the VLA D configuration.
(1 data file).

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