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Radio and X-ray Study of SNRs in the Magellanic Clouds

Published online by Cambridge University Press:  25 May 2016

M.D. Filipović ,
W. Pietsch ,
G. L. White ,
F. Haberl ,
L. Staveley-Smith ,
P. A. Jones ,
R. F. Haynes  and
M. Sasaki
M.D. Filipović
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Garching, Germany University of Western Sydney, Nepean, NSW 2747, Australia Australia Telescope National Facility, CSIRO, NSW 2121, Australia
W. Pietsch
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Garching, Germany
G. L. White
Affiliation:
University of Western Sydney, Nepean, NSW 2747, Australia
F. Haberl
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Garching, Germany
L. Staveley-Smith
Affiliation:
Australia Telescope National Facility, CSIRO, NSW 2121, Australia
P. A. Jones
Affiliation:
University of Western Sydney, Nepean, NSW 2747, Australia
R. F. Haynes
Affiliation:
Australia Telescope National Facility, CSIRO, NSW 2121, Australia
M. Sasaki
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Garching, Germany

Abstract

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We present our high-resolution radio-continuum and X-ray study of supernova remnants (SNRs) in the Magellanic Clouds (MCs). These investigations are based on Australia Telescope Compact Array (ATCA) radio-continuum and ROSAT X-ray observations. Our main aim is to study a complete sample of the MC SNRs and H II regions.

Type
Part 2: The Database
Information
Symposium - International Astronomical Union , Volume 192: The Stellar Content of Local Group Galaxies , 1999 , pp. 104 - 107
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

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