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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
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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.

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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. 2001-07-10. PSR J1016-5857: a young radio pulsar with possible supernova remnant, X-ray, and gamma-ray associations. https://doi.org/10.1086/323171

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