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A Deep Search for Young Pulsars in the Galactic Plane at 1400 MHz

Published online by Cambridge University Press:  04 August 2017

T.R. Clifton ,
A.W. Jones  and
A.G. Lyne
T.R. Clifton
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, United Kingdom
A.W. Jones
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, United Kingdom
A.G. Lyne
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield, Cheshire SK11 9DL, United Kingdom

Abstract

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A new survey of the Galactic plane for pulsars has now been completed at Jodrell Bank at the relatively high frequency of 1400 MHz (Clifton, T.R. and Lyne, A.G. 1986, Nature, 320, 43). A further 8 new objects have been detected. The properties of these are summarized below.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 47
Copyright
Copyright © Reidel 1987