Discovery of Diffuse Hard X-Ray Emission from the Vicinity of PSR J1648-4611 with Suzaku

作者：Sakai Michito^*; Matsumoto Hironori; Haba Yoshito; Kanou Yasufumi; Miyamoto Youhei

来源：Publications of the Astronomical Society of Japan, 2013, 65(3): UNSP 64.

DOI：10.1093/pasj/65.3.64

• acceleration of particles
• X-rays: individual (PSR J1648-4611, HESS J1646-458)

We observed the pulsar PSR J1648-4611 with Suzaku. Two X-ray sources, Suzaku J1648-4610 (Src A) and Suzaku J1648-4615 (Src B), were found in the field of view. Src A is coincident with the pulsar PSR J1648-4611, which was also detected by the Fermi Gamma-ray Space Telescope. A hard-band image indicates that Src A is spatially extended. We found point sources in the vicinity of Src A by using a Chandra image of the same region, but the point sources have soft X-ray emission, and cannot explain the hard X-ray emission of Src A. The hard-band spectrum of Src A can be reproduced by a power-law model with a photon index of 2.0(-0.7)(+0.9). The X-ray flux in the 2-10 keV band is 1.4 x 10(-13) erg cm(-2) s(-1). The diffuse emission suggests a pulsar wind nebula around PSR J1648-4611, but the luminosity of Src A is much larger than that expected from the spin-down luminosity of the pulsar. Parts of the very-high-energy gamma-ray emission of HESS J1646-458 may be powered by this pulsar wind nebula driven by PSR J1648-4611. Src B has soft emission, and its X-ray spectrum can be described by a power-law model with a photon index of 3.0(-0.8)(+1.4). The X-ray flux in the 0.4-10 keV band is 6.4 x 10(-14) erg s(-1) cm(-2). No counterpart for Src B has been found in the literature.

• 出版日期2013-6-25