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19 April 2024 |
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A radio supernova remnant associated with the young pulsar J1119-6127 | | Fronefield Crawford
; B. M. Gaensler
; V. M. Kaspi
; R. N. Manchester
; F. Camilo
; A. G. Lyne
; M. J. Pivovaroff
; | | Date: |
13 Dec 2000 | | Subject: | astro-ph | | Affiliation: | 1, 2), R. N. Manchester , F. Camilo , A. G. Lyne , M. J. Pivovaroff ( MIT, McGill, ATNF, Columbia, Jodrell Bank | | Abstract: | We report on Australia Telescope Compact Array observations in the direction of the young high magnetic-field pulsar J1119-6127. In the resulting images we identify a non-thermal radio shell of diameter 15’, which we classify as a previously uncatalogued young supernova remnant, G292.2-0.5. This supernova remnant is positionally coincident with PSR J1119-6127, and we conclude that the two objects are physically associated. No radio emission is detected from any pulsar wind nebula (PWN) associated with the pulsar; our observed upper limits are consistent with the expectation that high magnetic-field pulsars produce radio nebulae which fade rapidly. This system suggests a possible explanation for the lack of an associated radio pulsar and/or PWN in many supernova remnants. | | Source: | arXiv, astro-ph/0012287 | | Services: | Forum | Review | PDF | Favorites | |
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