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20 Pairs of Real Pulsar/Supernova Remnant Associations

Published online by Cambridge University Press:  19 July 2016

Wenwu Tian  and
Denis Leahy
Wenwu Tian
Affiliation:
National Astronomical Observatories, CAS, Beijing 100012, China Department of Physics & Astronomy, University of Calgary, Canada
Denis Leahy
Affiliation:
Department of Physics & Astronomy, University of Calgary, Calgary, T2N 1N4, Canada

Abstract

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We trace all pulsar/SNR associations proposed in the literature, and find that 20 pairs of associations are highly likely real because the pulsar wind nebulae around the pulsars have been detected.

Information

Type
Part 3: Pulsars: Surveys and Galactic Distribution
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 137 - 138
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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