SIMBAD references

2001ApJ...554..161P - Astrophys. J., 554, 161-172 (2001/June-2)

X-ray observations of the new pulsar-supernova remnant system PSR J1119-6127 and supernova remnant G292.2-0.5.

PIVOVAROFF M.J., KASPI V.M., CAMILO F., GAENSLER B.M. and CRAWFORD F.

Abstract (from CDS):

PSR J1119-6127 is a recently discovered 1600-yr-old radio pulsar that has a very high inferred surface dipolar magnetic field. We present a detailed analysis of a pointed ASCA observation and archival ROSAT data of PSR J1119-6127 and its surroundings. Both data sets reveal extended emission coincident with the newly discovered radio supernova remnant G292.2-0.5, which is reported in a companion paper by Crawford et al. A hard point source, offset ∼1'.5 from the position of the radio pulsar, is seen with the ASCA Gas Imaging Spectrometer (GIS). No pulsations are detected at the radio period with a pulsed fraction upper limit of 61% (95% confidence). The limited statistics prevent a detailed spectral analysis, although a power-law model with photon index Γ~1-2 describes the data well. Both the spectral model and derived X-ray luminosity are consistent with those measured for other young radio pulsars, although the spatial offset renders an identification of the source as the X-ray counterpart of the pulsar uncertain.

Abstract Copyright:

Journal keyword(s): ISM: individual (G292.2-0.5, AX J1119.1-6128.5) - pulsars: individual (J1119-6127) - Stars: Neutron - ISM: Supernova Remnants - X-Rays: Stars

CDS comments: p. 169 : IRAS J11169-6111 misprint for IRAS 11169-6111 (1950 coordinates)

Simbad objects: 19

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2020.02.29-12:09:25

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