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Physical processes in pulsar magnetospheres and non-thermal high-frequency emission
Published online by Cambridge University Press: 12 April 2016
Abstract
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The energy source of a pulsar’s non-thermal emission is the rotational energy loss of the neutron star. The rotational energy of the neutron star is transformed into the pulsar radiation by a long sequence of processes. The processes of this sequence are discussed.
- Type
- Part 5 High Energy Phenomena
- Information
- International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 323 - 330
- Copyright
- Copyright © Astronomical Society of the Pacific 1996
References
Thompson, D.J.
1994, in Second Compton Symposium, eds. Fichtel, C.E., N.Gehrels, , and Noris, J.P., AIP, 304, 57
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