activity
20082021
most citedNo anti-correlation between cyclotron line energy and X-ray flux in 4U 0115+634

88 citations · 540 across the 20 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2021

Chandra/LETGS Studies of the Collisional Plasma in 4U 1626-67

Paul B. Hemphill, Norbert S. Schulz, Herman M. Marshall +1

We present an analysis of \chandra/LETGS observations of the ultracompact X-ray binary (UCXB) 4U 162667, continuing our project to analyze the existing Chandra gratings data of…

astro-ph.HE2020★ 6 cited

NuSTAR observation of GRO J1744-28 at low mass accretion rate

O. König, F. Fürst, P. Kretschmar +8

We present the spectral analysis of the LMXB GRO J1744-28 using 29 ks of NuSTAR data taken in 2017 February at a low luminosity of erg/s (3-50 keV). The c…

astro-ph.HE2020★ 81 cited

Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions

Peter Kretschmar, Felix Fürst, Lara Sidoli +48

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology,…

astro-ph.HE2019★ 11 cited

The giant outburst of 4U 0115+634 in 2011 with Suzaku and RXTE

Matthias Bissinger né Kühnel, Ingo Kreykenbohm, Carlo Ferrigno +19

We present an analysis of X-ray spectra of the high mass X-ray binary 4U 0115+634 as observed with Suzaku and RXTE in 2011 July, during the fading phase of a giant X-ray outburst.…

astro-ph.HE2019★ 26 cited

Spectral and Timing Analysis of the accretion-powered pulsar 4U 1626-67 observed with Suzaku and NuSTAR

Wataru B. Iwakiri, Katja Pottschmidt, Sebastian Falkner +13

We present an analysis of the spectral shape and pulse profile of the accretion-powered pulsar 4U 1626-67 observed with Suzaku and NuSTAR during a spin-up state. The pulsar, which…

astro-ph.HE2019

The Physics of Accretion Onto Highly Magnetized Neutron Stars

Michael T. Wolff, Peter A. Becker, Joel Coley +16

Studying the physical processes occurring in the region just above the magnetic poles of strongly magnetized, accreting binary neutron stars is essential to our understanding of st…