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A Shell SNR Associated with PSR1930+22?

Published online by Cambridge University Press:  12 April 2016

D. Routledge  and
J.F. Vaneldik
D. Routledge
Affiliation:
University of Alberta, Edmonton, Canada
J.F. Vaneldik
Affiliation:
University of Alberta, Edmonton, Canada

Abstract

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Observations at 408 and 1420 MHz are reported which show a large (1.7 degree diameter) faint shell of nonthermal emission partially surrounding PSR1930+22. This may be the SNR associated with the pulsar, whose spin-down age is only 40000 years.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 339 - 342
Copyright
Copyright © Cambridge University Press 1988

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