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Supernova Remnant CTB 80 and PSR 1951+32

Published online by Cambridge University Press:  12 April 2016

R. G. Strom  and
B. W. Stappers
R. G. Strom
Affiliation:
NFRA, Radiosterrenwacht, Postbus 2, Dwingeloo, Netherlands Astronomical Institute, University of Amsterdam, Netherlands
B. W. Stappers
Affiliation:
Astronomical Institute, University of Amsterdam, Netherlands

Abstract

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The 39.5 ms pulsar PSR 1951+32 and the remnant with which it is associated, CTB 80, have both been observed with the recently upgraded Westerbork synthesis array (WSRT). Parts of CTB 80 have been observed over the frequency coverage from 0.3 to 8 GHz, while PSR 1951+32 has been observed from 0.3 to 1.6 GHz. The results are described and discussed in the context of the pulsar-remnant association.

Type
Part 7. The Surrounding of Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 509 - 512
Copyright
Copyright © Astronomical Society of the Pacific 2000

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