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Radio pulsars in the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

D. Mcconnell ,
P.M. Mcculloch ,
P.A. Hamilton ,
J.G. Ables ,
P.J. Hall ,
C.E. Jacka  and
A.J. Hunt
D. Mcconnell
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 94, Narrabri, NSW 2390, Australia
P.M. Mcculloch
Affiliation:
Department of Physics, University of Tasmania, PO Box 252C, Hobart, Tas., Australia
P.A. Hamilton
Affiliation:
Department of Physics, University of Tasmania, PO Box 252C, Hobart, Tas., Australia
J.G. Ables
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121, Australia
P.J. Hall
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 94, Narrabri, NSW 2390, Australia
C.E. Jacka
Affiliation:
Division of Radiophysics, CSIRO, PO Box 76, Epping, NSW 2121, Australia
A.J. Hunt
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 276, Parkes, NSW 2870, Australia

Abstract

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The Large Magellanic Cloud (LMC) and Small Magellanic Cloud (SMC) have been searched for radio pulsars using the 64-m Parkes radiotelescope. The search has resulted in the discovery of four pulsars. Observed dispersion measures to each suggest that three lie in the Clouds (two in the LMC, one in the SMC) and that the fourth, which was found in the direction of the LMC, is a foreground object belonging to the galactic pulsar population.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 322
Copyright
Copyright © Kluwer 1991