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Isolated neutron stars

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 06 Apr 2006Embargo end date: 01 Jan 2004Publisher:Cambridge University Press (CUP)

Authors: Mallory S. E. Roberts; Alice K. Harding; Victoria M. Kaspi;

doi: 10.1017/cbo9780511536281.008 , 10.48550/arxiv.astro-ph/0402136

arXiv: http://arxiv.org/abs/astro-ph/0402136

Isolated neutron stars

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Abstract

66 pages, 17 figures. To appear in "Compact Stellar X-ray Sources", eds. W.H.G. Lewin and M. van der Klis. High resolution images and Tables 8.1 and 8.2 available at http://www.physics.mcgill.ca/~vkaspi/isolated_neutron_stars

This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae.

Related Organizations

McGill University
Canada
Goddard Space Flight Center
United States
ROYAL INSTITUTION FOR THE ADVANCEMENT OF LEARNING MCGILL UNIVERSITY
Canada

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

Impact byBIP!

	citations This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	82
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Top 10%
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Top 10%
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Top 1%