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How well are Neutron Stars understood?

Published online by Cambridge University Press:  12 April 2016

Wolfgang Kundt
Wolfgang Kundt*
Affiliation:
Inst. f. Astroph. der Universität, Auf dem Hügel 71, D-53121Bonn

Abstract

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Alternative ways are discussed in which pulsars may (1) drive their winds, (2) avoid net electric currents, (3) emit coherent radio pulses, (4) acquire high spin rates, and (5) deal with moderate surface magnetic fields: 1011 < B/G ≲ 1014.

Type
Part 9. Population and Neutron Star Properties
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 597 - 598
Copyright
Copyright © Astronomical Society of the Pacific 2000

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