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Orbital Decay and Evidence of Disk Formation in the X-ray Binary Pulsar OAO 1657-415
P. A. Jenke, M. H. Finger, C. A. Wilson-Hodge +1
OAO 1657-415 is an eclipsing X-ray binary wind-fed pulsar that has exhibited smooth spin-up/spin-down episodes and has undergone several torque reversals throughout its long histor…
A Suzaku View of Cyclotron Line Sources and Candidates
K. Pottschmidt, S. Suchy, E. Rivers +20
Seventeen accreting neutron star pulsars, mostly high mass X-ray binaries with half of them Be-type transients, are known to exhibit Cyclotron Resonance Scattering Features (CRSFs)…
GBM Monitoring of Cyg X-1 During the Recent State Transition
G. L. Case, S. Baldridge, M. L. Cherry +5
Cygnus X-1 is a high-mass x-ray binary with a black hole compact object. It is normally extremely bright in hard x-rays and low energy gamma rays and resides in the canonical hard…
4U 1626-67 as seen by Suzaku before and after the 2008 torque reversal
A. Camero-Arranz, K. Pottschmidt, M. H. Finger +3
Aims. The accretion-powered pulsar 4U 1626-67 experienced a new torque reversal at the beginning of 2008, after about 18 years of steadily spinning down. The main goal of the prese…
X-Ray and Optical Observations of A 0535+26
A. Camero-Arranz, M. H. Finger, C. A. Wilson-Hodge +13
We present recent contemporaneous X-ray and optical observations of the Be/X-ray binary system A\,0535+26 with the \textit{Fermi}/Gamma-ray Burst Monitor (GBM) and several ground-b…
The Be/X-ray binary A0535+26 during its recent 2009/2010 outbursts
I. Caballero, K. Pottschmidt, A. Santangelo +20
The Be/X-ray binary A0535+26 showed a giant outburst in December 2009 that reached ~5.14 Crab in the 15-50 keV range. Unfortunately, due to Sun constraints it could not be observed…