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Do We Expect to See Young Pulsars outside Their Parent Shells?

Published online by Cambridge University Press:  25 April 2016

B. M. Gaensler  and
Simon Johnston
B. M. Gaensler
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia. simonj@physics.vsyd.edu.au
Simon Johnston
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia. simonj@physics.vsyd.edu.au
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Abstract

A recent study has indicated that a substantial fraction of young pulsars born in supernovae have travelled outside the boundaries of their corresponding shell supernova remnants. A simple model suggests that this should not be the case, implying either that some postulated pulsar/remnant associations are false, or that pulsars are particularly difficult to detect until they have emerged from their remnants.

Keywords

starsstatistics — starspulsarsgeneral — starssupernovaegeneral
Type
Gallactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 12 , Issue 1 , April 1995 , pp. 76 - 80
Copyright
Copyright © Astronomical Society of Australia 1995

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