SIMBAD references

2001ApJ...554..152C - Astrophys. J., 554, 152-160 (2001/June-2)

A radio supernova remnant associated with the young pulsar J1119-6127.

CRAWFORD F., GAENSLER B.M., KASPI V.M., MANCHESTER R.N., CAMILO F., LYNE A.G. and PIVOVAROFF M.J.

Abstract (from CDS):

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 nonthermal radio shell of diameter 15', which we classify as a previously uncataloged 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 that fade rapidly. This system suggests a possible explanation for the lack of an associated radio pulsar and/or PWN in many supernova remnants.

Abstract Copyright:

Journal keyword(s): ISM: Individual: Alphanumeric: G292.2-0.5 - Stars: Pulsars: Individual: Alphanumeric: PSR J1119-6127 - Radio Continuum: ISM - Stars: Neutron - ISM: Supernova Remnants

Status at CDS:  

CDS comments: p. 155 : IRAS J11169-6111 misprint for IRAS 11169-6111 (1950 coordinates)

Simbad objects: 24

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