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arXiv · astro-ph/0603017

Radio and infrared recombination studies of the southern massive star-forming region G333.6-0.2

Takuya Fujiyoshi·Craig H. Smith·James L. Caswell·Toby J. T. Moore·Stuart L. Lumsden·David K. Aitken·Patrick F. Roche
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Abstract

We present high spatial resolution radio and near-infrared hydrogen recombination line observations of the southern massive star-forming region G333.6-0.2. The 3.4-cm continuum peak is found slightly offset from the infrared source. The H90alpha spectra show for the first time a double peak profile at some positions. The complex velocity structure may be accounted for by champagne outflows, which may also explain the offset between the radio and infrared sources. The 2.17-um Brackett gamma image and H90alpha map are combined to construct an extinction map which shows a trend probably set by the blister nature of the HII region. The total number of Lyman continuum photons in the central 50-arcsec is estimated to be equivalent to that emitted by up to 19 O7V stars.

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Takuya Fujiyoshi, Craig H. Smith, James L. Caswell, Toby J. T. Moore, Stuart L. Lumsden, David K. Aitken, Patrick F. Roche. 2006-03-01. Radio and infrared recombination studies of the southern massive star-forming region G333.6-0.2. https://doi.org/10.1111/j.1365-2966.2006.10255.x

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