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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.

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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