activity
20072022
most citedPulse phase resolved analysis of the HMXB Cen X-3 over two binary orbits

93 citations · 970 across the 27 of their papers we have counts for

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Showing 2011Show all

8 papers · 1 filter

astro-ph.HE2011★ 47 cited

Study of the many fluorescent lines and the absorption variability in GX 301-2 with XMM-Newton

F. Fuerst, S. Suchy, I. Kreykenbohm +7

We present an in-depth study of the High Mass X-ray Binary (HMXB) GX 301-2 during its pre-periastron flare using data from the XMM-Newton satellite. The energy spectrum shows a pow…

astro-ph.HE2011★ 25 cited

Extended hard X-ray emission from the Vela pulsar wind nebula

Fabio Mattana, Diego Götz, Régis Terrier +8

The nebula powered by the Vela pulsar is one of the best examples of an evolved pulsar wind nebula, allowing to access the particle injection history and the interaction with the s…

astro-ph.HE2011★ 51 cited

Broadband spectroscopy using two Suzaku observation of the HMXB GX 301-2

Slawomir Suchy, Felix Fuerst, Katja Pottschmidt +5

We present the analysis of two Suzaku observations of GX 301-2 at two orbital phases after the periastron passage. Variations in the column density of the line-of-sight absorber ar…

astro-ph.HE2011★ 8 cited

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)…

astro-ph.HE2011★ 49 cited

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…

astro-ph.HE2011

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…