Modelling the multiwavelength light curves of PSR B1259−63/SS 2883

PSR B1259−63/SS 2883 is a binary system in which a 48-ms pulsar orbits around a Be star in a high-eccentric orbit with a long orbital period of about 3.4 yr. Extensive broad-band observational data are available for this system from the radio band to very high energy (VHE) range. The multifrequency...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2011-09, Vol.416 (2), p.1067-1076
Hauptverfasser:	Kong, S. W., Yu, Y. W., Huang, Y. F., Cheng, K. S.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Earth, ocean, space Exact sciences and technology Mathematical models Orbits pulsars: individual: PSR B1259−63 Stars & galaxies X-rays: binaries
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