Hostname: page-component-586b7cd67f-dlnhk Total loading time: 0 Render date: 2024-11-26T02:30:23.189Z Has data issue: false hasContentIssue false
  • English
  • Français

A VLA Survey for Radio Pulsars in the Galactic Center

Published online by Cambridge University Press:  12 April 2016

T. Joseph W. Lazio  and
James M. Cordes
T. Joseph W. Lazio
Affiliation:
Naval Research Laboratory, Code 7213, Washington, DC 20375-5351, USA
James M. Cordes
Affiliation:
Department of Astronomy, Cornell University and National Astronomy & Ionosphere Center, Ithaca, NY 14853-6801, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A radio pulsar in the Galactic center will suffer 350 seconds of pulse broadening. An imaging search for compact sources is far less desensitized by angular broadening than a periodicity search is affected by pulse broadening. We have conducted an imaging survey of the GC using the VLA and have detected approximately 200 sources. Six compact, steep-spectrum sources have been identified; additional compact sources with no spectral information have also been identified. Additional observations are in progress.

Type
Part 1. Searching for Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 39 - 40
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Becker, R.H., White, R.L., Helfand, D.J., & Zoonematkermani, S. 1994, ApJS, 91, 347 Google Scholar
Cordes, J.M. & Lazio, T.J.W. 1997, ApJ, 475, 557 Google Scholar
Frail, D.A., Diamond, P.J., Cordes, J.M., & van Langevelde, H.J. 1994, ApJ, 427, L43 Google Scholar
van Langevelde, H.J., Frail, D.A., Cordes, J.M., & Diamond, P.J. 1992, ApJ, 396, 686 Google Scholar
Yusef-Zadeh, F., Cotton, W., et al. 1994, ApJ, 434, L63 CrossRefGoogle Scholar