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26 April 2024
 
  » arxiv » astro-ph/0401472

 Article overview



An X-Ray Pulsar, Metal-rich Ejecta, and Shocked Ambient Medium in the Supernova Remnant G292.0+1.8
John P. Hughes ; Robert B. Friedman ; Patrick Slane ; Sangwook Park ;
Date 22 Dec 2003
Subject astro-ph
Affiliation1,2), Patrick Slane , and Sangwook Park ( Rutgers University, University of Chicago, Harvard-Smithsonian CfA, Pennsylvania State University
AbstractWe report the discovery of pulsed X-ray emission from the compact object CXOU J112439.1-591620 within the Galactic supernova remnant G292.0+1.8 using the High Resolution Camera on the Chandra X-Ray Observatory. The X-ray period is consistent with the extrapolation of the radio period and spindown rate of PSR J1124-5916. The X-ray pulse is single peaked and broad. There is no optical counterpart to a limit of M_V ~ 26. The pressure in the pulsar wind nebula is considerably less than that in the reverse-shock-heated ejecta and circumstellar medium, indicating that the reverse shock has not yet begun to interact with the nebula.
Source arXiv, astro-ph/0401472
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