Evolution of the Magnetic Field Structure of the Crab Pulsar-Reference-Cited by-同舟云学术

Evolution of the Magnetic Field Structure of the Crab Pulsar

Published:2013-11 Issue:6158 Volume:342 Page:598-601
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Lyne Andrew¹,Graham-Smith Francis¹,Weltevrede Patrick¹,Jordan Christine¹,Stappers Ben¹,Bassa Cees¹,Kramer Michael¹²

Affiliation:

1. Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester, M13 9PL, UK.

2. Max Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany.

Abstract

Magnetic Crab Since pulsars—highly magnetized rotating neutron stars—were discovered 45 years ago, the evolution of their magnetic field structure has been subject to much theoretical conjecture. However, observational evidence has been sparse. Now Lyne et al. (p. 598 ) report high-precision measurements, spanning more than two decades, that reveal the systematic evolution of the radiation pattern of the pulsar in the Crab Nebula, one of the youngest neutron stars known.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference29 articles.

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