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Search for an Optical Counterpart of PSR J0537–69101

Published online by Cambridge University Press:  12 April 2016

Christian Gouiffès  and
Hakki Ögelman
Christian Gouiffès
Affiliation:
Service d’Astrophysique, CEA/DSM/DAPNIA, C.E. Saclay, 91191 Gif-sur-Yvette Cedex, FRANCE, e-mail: [email protected]
Hakki Ögelman
Affiliation:
Department of Physics, University of Wisconsin, Madison, WI 53706, U.S.A, e-mail: [email protected]

Abstract

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We have conducted an optical study of the recently discovered very fast (P∼16msec) X-ray pulsar PSR J0537-6910 in the supernova remnant N157B. Broad band imaging has been obtained to study the field around the X-ray position and a high speed photometry programme was carried out in an attempt to detect optical pulses.

Type
Part 4. Optical Observations
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 301 - 302
Copyright
Copyright © Astronomical Society of the Pacific 2000

Footnotes

1

Based on data collected at the European Southern Observatory, La Silla, Chile.

References

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