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How well are Neutron Stars understood?
Published online by Cambridge University Press: 12 April 2016
Abstract
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