X-ray properties of the mode-switching pulsar PSR B0943+10
作者： S Mereghetti , L Kuiper , A Tiengo , J Hessels , W Hermsen
DOI: 10.1088/1742-6596/932/1/012009
关键词: Pulsar 、 Astrophysics 、 Intensity (heat transfer) 、 Physics 、 Radio telescope 、 X-ray 、 Flux 、 LOFAR 、 Radio spectrum 、 Magnetic field
摘要: The mode-switching pulsar PSR B0943+10 has been extensively studied in the radio band for many years and, more recently, it found to vary also X-rays, with a flux anticorrelated emission. Here we review results of long observations carried out XMM-Newton and LOFAR, LWA Arecibo telescopes 2014. These support scenario which both unpulsed non-thermal emission, likely magnetospheric origin, pulsed thermal emission from small polar cap (~1500 m2) strong non-dipolar magnetic field (~ 1014 G), are present during modes intensity correlated way.
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