activity
20092026
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 5.3k across the 102 of their papers we have counts for

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Showing 2017Show all

11 papers · 1 filter

astro-ph.HE2017★ 21 cited

Spectral and Timing Properties of IGR J17091-3624 in the Rising Hard State During its 2016 Outburst

Yanjun Xu, Javier A. Garcia, Felix Fuerst +8

We present a spectral and timing study of the NuSTAR and Swift observations of the black hole candidate IGR J17091-3624 in the hard state during its outburst in 2016. Disk reflecti…

astro-ph.HE2017★ 80 cited

Reflection Spectra of the Black Hole Binary Candidate MAXI J1535-571 in the Hard State Observed by NuSTAR

Yanjun Xu, Fiona A. Harrison, Javier A. Garcia +9

We report on a NuSTAR observation of the recently discovered bright black hole candidate MAXI J1535-571. NuSTAR observed the source on MJD 58003 (five days after the outburst was r…

astro-ph.HE2017★ 23 cited

Inversion of the decay of the cyclotron line energy in Her X-1

R. Staubert, D. Klochkov, F. Fürst +3

Recent observations of Her X-1 with NuSTAR and INTEGRAL in 2016 have provided evidence that the 20-year decay of the cyclotron line energy found between 1996 and 2015 has ended and…

astro-ph.IM2017★ 14 cited

Paving the way to simultaneous multi-wavelength astronomy

M. J. Middleton, P. Casella, P. Gandhi +49

Whilst astronomy as a science is historically founded on observations at optical wavelengths, studying the Universe in other bands has yielded remarkable discoveries, from pulsars…

astro-ph.HE2017★ 53 cited

NuSTAR Resolves the First Dual AGN above 10 keV in SWIFT J2028.5+2543

Michael J. Koss, Ana Glidden, Mislav Balokovic +19

We have discovered heavy obscuration in the dual active galactic nucleus (AGN) in the Swift/Burst Alert Telescope (BAT) source SWIFT J2028.5+2543 using Nuclear Spectroscopic Telesc…

astro-ph.HE2017★ 18 cited

An XMM-Newton and NuSTAR study of IGR J18214-1318: a non-pulsating high-mass X-ray binary with a neutron star

Francesca M. Fornasini, John A. Tomsick, Matteo Bachetti +5

IGR J18214-1318, a Galactic source discovered by the International Gamma-Ray Astrophysics Laboratory, is a high-mass X-ray binary (HMXB) with a supergiant O-type stellar donor. We…

astro-ph.HE2017★ 78 cited

Super-Eddington Accretion onto the Neutron Star NGC 7793 P13: Broadband X-ray Spectroscopy and Ultraluminous X-ray Sources

D. J. Walton, F. Fuerst, F. A. Harrison +8

We present a detailed, broadband X-ray spectral analysis of the ULX pulsar NGC 7793 P13, a known super-Eddington source, utilizing data from the -, and $Chand…

astro-ph.SR2017★ 22 cited

Spectroscopic twin to the hypervelocity sdO star US 708 and three fast sdB stars from the Hyper-MUCHFUSS project

E. Ziegerer, U. Heber, S. Geier +4

Important tracers for the dark matter halo of the Galaxy are hypervelocity stars (HVSs), which are faster than the local escape velocity of the Galaxy and their slower counterparts…

astro-ph.HE2017

Stellar Winds in Massive X-ray Binaries

Peter Kretschmar, Silvia Martínez-Núñez, Enrico Bozzo +15

Strong winds from massive stars are a topic of interest to a wide range of astrophysical fields. In High-Mass X-ray Binaries the presence of an accreting compact object on the one…

astro-ph.HE2017★ 49 cited

Cyclotron resonant scattering feature simulations. II. Description of the CRSF simulation process

F. -W. Schwarm, R. Ballhausen, S. Falkner +12

Cyclotron resonant scattering features (CRSFs) are formed by scattering of X-ray photons off quantized plasma electrons in the strong magnetic field (of the order 10^12 G) close to…

astro-ph.HE2017★ 144 cited

Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries

Silvia Martínez-Núñez, Peter Kretschmar, Enrico Bozzo +13

Massive stars, at least 10 times more massive than the Sun, have two key properties that make them the main drivers of evolution of star clusters, galaxies, and the Universe…