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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1579

Title: Electron temperatures in the galactic HII regions W43 and M17
Authors: Subrahmanyan, Ravi
Goss, W.M.
Keywords: HII REGIONS,
ISM: INDIVIDUAL: M17,
ISM: INDIVIDUAL: W43,
RADIO CONTINUUM: ISM
Issue Date: Jul-1996
Publisher: Blackwell Publishing for the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, 1996, Vol.281, p 239-244
Abstract: We present 1.2-arcmin resolution images of the Galactic HII regions W43 and M17 made with the Very Large Array (VLA) at a frequency of 330 MHz; these are the highest resolution images to date of the large-scale structures of these complexes at any frequency. The electron temperature towards the component of W43 that has the highest emission measure, G30.8-0.0, is 5410+/-300K. The electron temperatures towards the components of M17, G15.0-0.7 and G15.1-0.7, are 7600^+700-210 and 8000^+450-220 K respectively. These estimates are consistent with previous estimates based on radio recombination line and continuum observations of these HII regions.
Description: Sorry, the full text of this article is not available here. Please click on the alternative location to access it.
URI: http://hdl.handle.net/2289/1579
ISSN: 0035-8711
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?1996MNRAS.281..239S
http://adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996MNRAS.281..239S&link_type=ARTICLE&db_key=AST
Copyright: (1996) Royal Astronomical Society
Appears in Collections:Research Papers (A&A)

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