Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Far-infrared and radio observations of the W31 star-forming region

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/168122· OSTI ID:7193705
; ; ; ;  [1]
  1. Tata Institute of Fundamental Research, Bombay (India)
New 150 micron mapping of the W31 star-forming region with a resolution of 1.5 arcmin has resolved 12 sources, including eight new ones. About 35 percent of the emission is of diffuse origin. The IRAS two-dimensional COADD data of the same region at 60 and 100 microns have been deconvolved using a maximum-entropy algorithm. The dust temperature, dust optical depth, far-IR luminosity, and so on, have been derived for individual sources in the star-forming complex; several of these seem to be excited by embedded young stars. One young stellar object with an optically thick ionized envelope has been identified. New high-resolution maps of selected regions around the two most prominent H II regions in the W31 complex, G10.2-0.3 and G10.3-0.1, have been obtained at 5 and 15 GHz using the VLA. The initial mass function for G10.2-0.3 is quite steep. An energetic bipolar outflow source candidate has been found which is proposed to be the mid-IR source in the G10.2-0.3 complex. 41 refs.
OSTI ID:
7193705
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 347; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English