INTEGRAL detection of the pulsar wind nebula in PSR J1846-0258
de Rosa, A.; Hill, A. B.; Bird, A. J.; McBride, V. A.; Landi, R.; Malizia, A.; Bazzano, A.; Dean, A. J.; Sguera, V.
United Kingdom, Italy
Abstract
Aims:We communicate the detection of soft (20-200 keV) γ-rays from the pulsar and pulsar wind nebula of PSR J1846-0258 and aim to identify the component of the system which is responsible for the γ-ray emission.
Methods: We combine spectral information from the INTEGRAL γ-ray mission with archival data from the Chandra X-ray Observatory to pinpoint the source of soft γ-ray emission.
Results: Our analysis shows that the soft γ-rays detected from PSR J1846-0258 include emission from both the pulsar and the pulsar wind nebula, but the measured spectral shape is dominated by the pulsar wind nebula. We discuss PSR J1846-0258 in the context of rotation-powered pulsars with high magnetic field strengths and review the anomalously high fraction of spin-down luminosity converted into X- and γ-ray emission in light of a possible overestimate of the distance to this pulsar.