No CrossRef data available.
Article contents
Physical processes in pulsar magnetospheres and non-thermal high-frequency emission
Published online by Cambridge University Press: 12 April 2016
Abstract
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