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New Pulsars Coincident with Unidentified Gamma-Ray Sources

Published online by Cambridge University Press:  19 July 2016

Mallory Roberts ,
Scott Ransom ,
Jason Hessels ,
Margaret Livingstone ,
Cindy Tam ,
Victoria Kaspi  and
Fronefield Crawford
Mallory Roberts
Affiliation:
Dept. of Physics, McGill University, Montréal, QC, H3A 2T8, Canada
Scott Ransom
Affiliation:
Dept. of Physics, McGill University, Montréal, QC, H3A 2T8, Canada
Jason Hessels
Affiliation:
Dept. of Physics, McGill University, Montréal, QC, H3A 2T8, Canada
Margaret Livingstone
Affiliation:
Dept. of Physics, McGill University, Montréal, QC, H3A 2T8, Canada
Cindy Tam
Affiliation:
Dept. of Physics, McGill University, Montréal, QC, H3A 2T8, Canada
Victoria Kaspi
Affiliation:
Dept. of Physics, McGill University, Montréal, QC, H3A 2T8, Canada
Fronefield Crawford
Affiliation:
Dept. of Physics, Haverford College, Haverford, PA 19041, USA

Abstract

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We present the results of radio searches for pulsars within unidentified EGRET source error boxes. Using the Parkes multibeam system, we have surveyed 56 sources at Galactic latitudes |b| > 5° which do not appear to be associated with blazars. This population has been suggested to be distributed like the local star forming region known as the Gould Belt, the Galactic Halo, and/or the millisecond pulsars. We have discovered several new pulsars in this survey, including three new binary systems.

Type
Part 9: Optical, X-ray and Gamma-ray Observations
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 415 - 418
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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