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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 | Abstract: | We 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 | Services: | Forum | Review | PDF | Favorites |
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