Discovery of synchronous X-ray and radio moding of PSR B0823+26

Abstract

Simultaneous observations of PSR B0823+26 with ESA's XMM-Newton, the Giant Metrewave Radio Telescope and international stations of the Low Frequency Array revealed synchronous X-ray/radio switching between a radio-bright (B) mode and a radio-quiet (Q) mode. During the B mode we detected PSR B0823+26 in 0.2-2 keV X-rays and discovered pulsed emission with a broad sinusoidal pulse, lagging the radiomain pulse by 0.208+/-0.012 in phase, with high pulsed fraction of 70-80%. During the Q mode PSR B0823+26 was not detected in X-rays (2sigma upper limit a factor ~9 below the B-mode flux). The total X-ray spectrum, pulse profile and pulsed fraction can globally be reproduced with a magnetized partially ionized hydrogen atmosphere model with three emission components: a primary small hot spot (T~3.6x10^6 K, R~17 m), a larger cooler concentric ring (T~1.1x10^6 K, R~280 m) and an antipodal hot spot (T~1.1x10^6 K, R~100 m), for the angle between the rotation axis and line of sight direction ~66deg. The latter is in conflict with the radio derived value of (84+/-0.7)deg. The average X-ray flux within hours-long B-mode intervals varied by a factor +/-20%, possibly correlated with variations in the frequency and lengths of short radio nulls or short durations of weak emission. The correlated X-ray/radio moding of PSR B0823+26 is compared with the anti-correlated moding of PSR B0943+10, and the lack of X-ray moding of PSR B1822-09. We speculate that the X-ray/radio switches of PSR B0823+26 are due to variations in the rate of accretion of material from the interstellar medium through which it is passing.

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ORCID for Wynn C.G. Ho: orcid.org/0000-0002-6089-6836

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