paper

Exploring the X-ray and gamma-ray properties of the redback millisecond pulsar PSR J1723-2837

arXiv:1311.0223 · doi:10.1088/2041-8205/781/1/L21

Abstract

We have investigated the X-ray and -ray properties of the redback millisecond pulsar PSR J1723-2837 with XMM-Newton, Chandra and Fermi. We have discovered the X-ray orbital modulation of this binary system with the minimum that coincides with the phases of radio eclipse. The X-ray emission is clearly non-thermal in nature which can be well described by a simple power-law with a photon index of . The phase-averaged luminosity is erg/s in 0.3-10 keV which consumes of the spin-down power. We have detected the ray emission in GeV from this system at a significance of for the first time. The rays in this energy range consumes of the spin-down power and can be modeled by a power-law with a photon index of . We discuss the high energy properties of the new redback in the context of a intrabinary shock model.

13 pages, 3 figures, accepted for publication in ApJ Letter

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