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Paper detail

A 0535+26: an X-ray/Optical Tour

We compiled X-ray and Optical observations of the accreting X-ray binary system A 0535+262 since its discovery in 1975, that will allow us to shed light on the unpredictable behavior of this binary system. We present the data in terms of the Be-disk interaction with the neutron star companion. In addition, we show recent results from the continuous monitoring of this source by the Gamma-ray Burst Monitor(GBM), on board the Fermi observatory, since its launch in 2008 June 11.

preprint2011arXivOpen access
A. Camero-ArranzM. H. FingerC. A. Wilson-HodgeP. JenkeM. J. CoeI. SteeleI. CaballeroJ. Gutierrez-SotoP. KretschmarJ. SusoV. A. McBrideJ. Rodriguez
astro-ph.HE
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A. Camero-ArranzM. H. FingerC. A. Wilson-HodgeP. JenkeM. J. CoeI. SteeleI. CaballeroJ. Gutierrez-SotoP. KretschmarJ. SusoV. A. McBrideJ. Rodriguez

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