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16 February 2025
 
  » arxiv » astro-ph/0107180

 Article overview



PSR J1016-5857: a young radio pulsar with possible supernova remnant, X-ray, and gamma-ray associations
F. Camilo ; J. F. Bell ; R. N. Manchester ; A. G. Lyne ; A. Possenti ; M. Kramer ; V. M. Kaspi ; I. H. Stairs ; N. D’Amico ; G. Hobbs ; E. V. Gotthelf ; B. M. Gaensler ;
Date 10 Jul 2001
Journal Astrophys.J. 557 (2001) L51
Subject astro-ph
Affiliation Columbia, ATNF, Jodrell Bank, Bologna, McGill, NRAO, MIT
AbstractWe report the discovery of a young and energetic pulsar in the Parkes multibeam survey of the Galactic plane. PSR J1016-5857 has a rotation period of 107 ms and period derivative of 8e-14, implying a characteristic age of 21 kyr and spin-down luminosity of 2.6e36 erg/s. The pulsar is located just outside, and possibly interacting with, the shell supernova remnant G284.3-1.8. Archival X-ray data show a source near the pulsar position which is consistent with emission from a pulsar wind nebula. The pulsar is also located inside the error box of the unidentified EGRET source 3EG J1013-5915, for which it represents a plausible counterpart.
Source arXiv, astro-ph/0107180
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