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Book Chapter

Energetic Radiation from Magnetized Neutron Stars

  • Ruderman M
Springer Netherlands, (1987), 145-191
DOI: 10.1007/978-94-009-3823-6_7
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Abstract

The author considers in detail the problems of the origin of the non-radio emission from the young isolated radiopulsars, effects from the evolution of neutron star properties (especially magnetic fields), and how these might lead to older neutron stars in accreting binaries becoming sources of superenergetic radiation. Especially, he discusses the non-radio emission from the Crab and Vela neutron stars.

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APA

Ruderman, M. A. (1987). Energetic Radiation from Magnetized Neutron Stars. In High Energy Phenomena Around Collapsed Stars (pp. 145–191). Springer Netherlands. https://doi.org/10.1007/978-94-009-3823-6_7

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