AbstractWe have analysed 9 years of data from the All Sky Monitor on the Rossi X-ray Timing Explorer for 2S 0114+650 to study the evolution of its spin, binary, and super-orbital periods. The spin history of the neutron star in this system exhibits torque reversals lasting ∼1 year. The newly discovered super-orbital period has remained stable over the 9-year span, making 2S 0114+650 the fourth known system to exhibit stable super-orbital modulation. We compare its super-orbital period evolution with those of the other three such systems.
Evolution of the periodicities in 2S 0114+650
Advances in Space Research ; 38 , 12 ; 2779-2781
2006-02-24
3 pages
Article (Journal)
Electronic Resource
English
X-rays , binary , Stars , neutron , Accretion , accretion discs , individual (2S 0114+650)
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