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Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae

Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1017984993

Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae

About this item

Full title

Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae

Publisher

Dordrecht: Springer Netherlands

Journal title

Space science reviews, 2012-05, Vol.166 (1-4), p.231-261

Language

English

Formats

Publication information

Publisher

Dordrecht: Springer Netherlands

More information

Scope and Contents

Contents

We review the observations of supernova remnants (SNRs) and pulsar-wind nebulae (PWNe) that give information on the strength and orientation of magnetic fields. Radio polarimetry gives the degree of order of magnetic fields, and the orientation of the ordered component. Many young shell supernova remnants show evidence for synchrotron X-ray emissio...

Alternative Titles

Full title

Magnetic Fields in Supernova Remnants and Pulsar-Wind Nebulae

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_1017984993

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1017984993

Other Identifiers

ISSN

0038-6308

E-ISSN

1572-9672

DOI

10.1007/s11214-011-9775-y

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