Supernova Remnants in the Large Magellanic Cloud
- 25 April 1994
- journal article
- invited
- Published by Cambridge University Press (CUP) in Publications of the Astronomical Society of Australia
- Vol. 11 (2) , 99-109
- https://doi.org/10.1017/s1323358000019780
Abstract
Twelve supernova remnants in the Large Magellanic Cloud have now been observed with the Australia Telescope. These were all imaged in total intensity and where possible the linear polarisation was also mapped. In many respects this survey is similar to previous single-dish observations of Galactic supernova remnants, and comparisons are made with these results. Preliminary images are shown for several sources. The survey is continuing with additional array configurations and at other wavelengths.Keywords
This publication has 16 references indexed in Scilit:
- Hidden supernova remnants in the Large Magellanic Cloud H II complex N44The Astrophysical Journal, 1993
- Radio emission from young supernova remnants. II - Evolution and dependence on characteristics of the progenitor and the external mediumThe Astrophysical Journal, 1993
- Radio structure of the remnant of Tycho's supernova (SN 1572)The Astronomical Journal, 1991
- Environments and populations of supernova remnants in the Large Magellanic CloudThe Astronomical Journal, 1988
- Echelle observations of supernova remnants in the Magellanic CloudsThe Astronomical Journal, 1988
- Statistical studies of supernova remnantsMonthly Notices of the Royal Astronomical Society, 1984
- A New Look at Radio Supernova RemnantsAustralian Journal of Physics, 1984
- Supernova remnants in the Large Magellanic CloudMonthly Notices of the Royal Astronomical Society, 1980
- Magnetic Fields in Supernova RemnantsAustralian Journal of Physics, 1976
- 5 GHz Polarization Observations of 33 Galactic Radio SourcesAustralian Journal of Physics, 1975