A new model for the X-ray continuum of the magnetized accreting pulsars

Context. Accreting highly magnetized pulsars in binary systems are among the brightest X-ray emitters in our Galaxy. Although a number of high-quality broad-band (0.1–100 keV) X-ray observations are available, the spectral energy distribution of these sources is usually investigated by adopting pure...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2016-07, Vol.591, p.A29
Hauptverfasser:	Farinelli, Ruben, Ferrigno, Carlo, Bozzo, Enrico, Becker, Peter A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Continuums Cyclotrons Emission analysis magnetic fields Mathematical models Neutron stars Pulsars pulsars: individual: 4U 0115+63 pulsars: individual: Cen X-3 pulsars: individual: Her X-1 radiative transfer X-rays X-rays: binaries
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