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.
Cite
@article{arxiv.1105.2081,
title = {A 0535+26: an X-ray/Optical Tour},
author = {A. Camero-Arranz and M. H. Finger and C. A. Wilson-Hodge and P. Jenke and M. J. Coe and I. Steele and I. Caballero and J. Gutierrez-Soto and P. Kretschmar and J. Suso and V. A. McBride and J. Rodriguez},
journal= {arXiv preprint arXiv:1105.2081},
year = {2015}
}
Comments
4 pages, 5 figures, Conference proceeding of "Astrophysics of Neutron Stars 2010 - a conference in honor of M. Ali Alpar", 2-6 August 2010, Cesme, Izmir, Turkey