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Bow Shocks from Radio Pulsars: Observations of the Guitar Nebula

Published online by Cambridge University Press:  12 April 2016

Shami Chatterjee  and
James M. Cordes
Shami Chatterjee
Affiliation:
Astronomy and Space Sciences, Cornell University, Ithaca, NY 14853
James M. Cordes
Affiliation:
Astronomy and Space Sciences, Cornell University, Ithaca, NY 14853

Abstract

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We present optical observations and radio non-detections of the bow shock nebula associated with the pulsar B2224+65 (the “Guitar Nebula”), and fit an analytic model to the observed bow shock to estimate its inclination and constrain other parameters (distance, pulsar velocity, ISM density). We also test scaling laws for bow shock parameters.

Type
Part 7. The Surrounding of Pulsars
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 517 - 518
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Cordes, J.M., Romani, R.W., & Lundgren, S.C. 1993, Nature, 362, 133 Google Scholar
Wilkin, F.P., ApJ, 459, L31 Google Scholar