PSR B1951+32: A Bow Shock-confined X-Ray Nebula, a Synchrotron Knot, and an Optical Counterpart Candidate-Reference-Cited by-同舟云学术

PSR B1951+32: A Bow Shock-confined X-Ray Nebula, a Synchrotron Knot, and an Optical Counterpart Candidate

Published:2004-06-22 Issue:1 Volume:610 Page:L33-L36
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Moon D.-S.,Lee J.-J.,Eikenberry S. S.,Koo B.-C.,Chatterjee S.,Kaplan D. L.,Hester J. J.,Cordes J. M.,Gallant Y. A.,Koch-Miramond L.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference15 articles.

1. Detection of new optical counterpart candidates to PSR B1951+32 with HST/WFPC2

2. Bow Shocks from Neutron Stars: Scaling Laws andHubble Space TelescopeObservations of the Guitar Nebula

3. A six year timing solution for PSR B1951 + 32

4. Gaensler, B. M., van der Swaluw, E., Camilo, F., Kaspi, V. M., Baganoff, F. K., Yusef-Zadeh, F. & Manchester, R. N. 2003, ApJ, submitted (astro-ph/0312362)

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