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Comparison of Discrete Sources in Radio and Hα Surveys of the Magellanic Clouds and the Potential for the New Hα Survey

Published online by Cambridge University Press:  16 May 2016

Miroslav D. Filipović ,
Paul A. Jones ,
Graeme L. White  and
Raymond F. Haynes
Miroslav D. Filipović*
Affiliation:
University of Western Sydney, Nepean, PO Box 10, Kingswood, NSW 2747, Australia Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse, D-85740, Germany Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia
Paul A. Jones
Affiliation:
University of Western Sydney, Nepean, PO Box 10, Kingswood, NSW 2747, Australia
Graeme L. White
Affiliation:
University of Western Sydney, Nepean, PO Box 10, Kingswood, NSW 2747, Australia
Raymond F. Haynes
Affiliation:
University of Western Sydney, Nepean, PO Box 10, Kingswood, NSW 2747, Australia Australia Telescope National Facility, CSIRO, PO Box 76, Epping, NSW 2121, Australia
*
M.Filipovic@nepean.uws.edu.au
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Abstract

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We present a comparison between the latest Parkes radio surveys (Filipović et al. 1995, 1996, 1997) and Hα surveys of the Magellanic Clouds (Kennicutt & Hodge 1986). We have found 180 discrete sources in common for the Large Magellanic Cloud (LMC) and 40 in the field of the Small Magellanic Cloud (SMC). Most of these sources (95%) are HII regions and supernova remnants (SNRs). A comparison of the radio and Hα flux densities shows a very good correlation and we note that many of the Magellanic Clouds SNRs are embedded in HII regions.

Keywords

galaxies: Magellanic Cloudsradio continuum: galaxiesISM: HII regionsISM: supernova remnants
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 15 , Issue 1 , 1998 , pp. 128 - 131
Copyright
Copyright © Astronomical Society of Australia 1998

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