High-Spatial Resolution Radio Observations of the Star-Forming Region G333.6-0.2

Details High-Spatial Resolution Radio Observations of the Star-Forming Region G333.6-0.2 High-Spatial Resolution Radio Observations of the Star-Forming Region G333.6-0.2

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..401f&link_type=abstract

Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam

Computer Science

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Scientific paper

Results from radio synthesis observations of the bright southern massive star-forming region G333.6-0.2 are presented. The overall morphology of high-spatial resolution (1.6 arcsec) 3.4-cm continuum and H90α radio recombination line (RRL) maps constructed is remarkably similar to the infrared (IR) images obtained at comparable spatial resolution. However, it is found that the radio continuum peak does not coincide with the IR main peak position, nor does it have any obvious IR counterparts. The H90α spectra reveal a complex velocity structure across the Hii region with some areas exhibiting double-peaked profiles. These findings could be explained by a scenario that involves bipolar outflows.

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