Radio and X-ray Properties of Magellanic Cloud Supernova Remnants

Details Radio and X-ray Properties of Magellanic Cloud Supernova Remnants Radio and X-ray Properties of Magellanic Cloud Supernova Remnants

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xrrc.proce4.04d&link_type=abstract

"X-Ray and Radio Connections (eds. L.O. Sjouwerman and K.K Dyer) Published electronically by NRAO, http://www.aoc.nrao.edu/event

Mathematics

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X-Ray, Radio, Supernova Remnants

Scientific paper

The Magellanic Clouds provides an invaluable sample of supernova remnants (SNRs) for comparative radio and X-ray morphological studies. The clouds contain a variety of remnants, all at the same distance. There are shell SNRs with thermal X-rays and non-thermal radio emission, pulsar wind nebulae (with and without observable pulsars) producing non-thermal radio and X-ray synchrotron emission, and composite objects containing both of these components. There are also mixed-morphology SNRs with shell radio emission and internal thermal X-rays. Often the X-ray and radio emission match well but sometimes they are surprisingly different in structure for reasons that are still being investigated.

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