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High-energy radiation from magnetized neutron stars

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Neutron stars, the most extreme state of matter yet confirmed, are responsible for much of the high-energy radiation detected in the universe. Meszaros provides a general overview of the physics of magnetized neutron stars, discusses in detail the radiation processes and transport properties relevant to the production and propagation of high-energy radiation in the outer layers of these objects, and reviews the observational properties and theoretical models of various types of neutron star sources.

Author(s): Peter Meszaros
Series: Theoretical Astrophysics
Publisher: UCP
Year: 1992

Language: English
Pages: 532