A deep campaign to characterize the synchronous radio/X-ray mode switching of PSR B0943+10

Abstract : We report on simultaneous X-ray and radio observations of the mode-switching pulsar PSR B0943+10 obtained with the XMM-Newton satellite and the LOFAR, LWA and Arecibo radio telescopes in November 2014. We confirm the synchronous X-ray/radio switching between a radio-bright (B) and a radio-quiet (Q) mode, in which the X-ray flux is a factor ∼ 2.4 higher than in the B-mode. We discovered X-ray pulsations, with pulsed fraction of 38±5% (0.5-2 keV), during the B-mode, and confirm their presence in Q-mode, where the pulsed fraction increases with energy from ∼20% up to ∼65% at 2 keV. We found marginal evidence for an increase in the X-ray pulsed fraction during B-mode on a timescale of hours. The Q-mode X-ray spectrum requires a fit with a two-component model (either a power-law plus blackbody or the sum of two blackbodies), while the B-mode spectrum is well fit by a single blackbody (a single power-law is rejected). With a maximum likelihood analysis, we found that in Q-mode the pulsed emission has a thermal blackbody spectrum with temperature ∼ 3.4 × 10 6 K and the unpulsed emission is a power-law with photon index ∼2.5, while during B-mode both the pulsed and unpulsed emission can be fit by either a blackbody or a power law with similar values of temperature and photon index. A Chandra image shows no evidence for diffuse X-ray emission. These results support a scenario in which both unpulsed non-thermal emission, likely of magnetospheric origin, and pulsed thermal emission from a small polar cap (∼1500 m 2) with a strong non-dipolar magnetic field (∼ 10 14 G), are present during both radio modes and vary in intensity in a correlated way. This is broadly consistent with the predictions of the partially screened gap model and does not necessarily imply global magnetospheric rearrangements to explain the mode switching.
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Soumis le : mardi 22 novembre 2016 - 10:35:24
Dernière modification le : jeudi 7 février 2019 - 17:03:33
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A Mereghetti, A Kuiper, P Tiengo, P Hessels, P Hermsen, et al.. A deep campaign to characterize the synchronous radio/X-ray mode switching of PSR B0943+10. Astrophysical Journal, American Astronomical Society, 2016, 831 (1), pp.21. 〈10.3847/0004-637X/831/1/21〉. 〈insu-01400553〉



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