activity
20122019
most citedDiscovery and Modeling of a Flattening of the Positive Cyclotron Line/Luminosity Relation in GX 304-1 with RXTE

50 citations · 108 across the 5 of their papers we have counts for

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5 papers · 1 filter

astro-ph.HE2019★ 2 cited

Variability in high-mass X-ray binaries

F. Fuerst, P. Kretschmar, V. Grinberg +5

Strongly magnetized, accreting neutron stars show periodic and aperiodic variability over a wide range of time scales. By obtaining spectral and timing information on these differe…

astro-ph.HE2017★ 18 cited

Studying the accretion geometry of EXO 2030+375 at luminosities close to the propeller regime

F. Fuerst, P. Kretschmar, J. J. E. Kajava +10

The Be X-ray binary EXO 2030+375 was in an extended low luminosity state during most of 2016. We observed this state with NuSTAR and Swift, supported by INTEGRAL observations as we…

astro-ph.HE2017★ 23 cited

A multi-wavelength study of SXP 1062, the long period X-ray pulsar associated with a supernova remnant

A. Gonzalez-Galan, L. M. Oskinova, S. B. Popov +5

SXP 1062 is a Be X-ray binary located in the Small Magellanic Cloud. It hosts a long-period X-ray pulsar and is likely associated with the supernova remnant MCSNR J0127-7332. In th…

astro-ph.HE2016★ 50 cited

Discovery and Modeling of a Flattening of the Positive Cyclotron Line/Luminosity Relation in GX 304-1 with RXTE

Richard E. Rothschild, Matthias Kuehnel, Katja Pottschmidt +8

The RXTE observed four outbursts of the accreting X-ray binary transient source, GX 304-1 in 2010 and 2011. We present results of detailed 3-100 keV spectral analysis of 69 separat…

astro-ph.HE2012★ 15 cited

Staring at 4U 1909+07 with Suzaku

F. Fuerst, K. Pottschmidt, I. Kreykenbohm +4

We present an analysis of the neutron star High Mass X-ray Binary (HMXB) 4U 1909+07 mainly based on Suzaku data. We extend the pulse period evolution, which behaves in a random-wal…