Friday, May 4, 2012

1205.0719 (R. de los Reyes et al.)

A newly discovered VHE gamma-ray PWN candidate around PSR J1459-60    [PDF]

R. de los Reyes, A. Zajczyk, R. C. G. Chaves, for the H. E. S. S. collaboration
Observations of the Galactic Plane performed by the H.E.S.S. telescope array have revealed a significant excess at very-high-energies (VHE; E>0.1 TeV) from the direction of PSR J1459-60, a rather old gamma-ray pulsar (64 kyr) with a spindown energy of ~10^36 erg/s, discovered by the Fermi/LAT satellite in high-energy (HE) gamma-rays. The X-ray pulsar counterpart has been recently detected using the Suzaku satellite. In this contribution, we present the discovery of a new VHE gamma-ray source, including morphological and spectral analyses. Its association with the gamma-ray pulsar in a PWN scenario will be discussed.
View original: http://arxiv.org/abs/1205.0719

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