Search Results - "Wilms, Jorn"
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The Effects of High Density on the X-ray Spectrum Reflected from Accretion Discs Around Black Holes
Published in Monthly notices of the Royal Astronomical Society (11-10-2016)“…Current models of the spectrum of X-rays reflected from accretion discs around black holes and other compact objects are commonly calculated assuming that the…”
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Reflection Spectroscopy of the Black Hole Binary XTE J1752−223 in Its Long-stable Hard State
Published in The Astrophysical journal (01-09-2018)“…We present a detailed spectral analysis of the black hole binary XTE J1752−223 in the hard state of its 2009 outburst. Regular monitoring of this source by the…”
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SPECTRAL STATE DEPENDENCE OF THE 0.4-2 MEV POLARIZED EMISSION IN CYGNUS X-1 SEEN WITH INTEGRAL/IBIS, AND LINKS WITH THE AMI RADIO DATA
Published in The Astrophysical journal (01-07-2015)“…ABSTRACT Polarization of the keV hard tail of the microquasar Cygnus X-1 has been independently reported by INTEGRAL/Imager on Board the INTEGRAL Satellite…”
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Modeling the Precession of the Warped Inner Accretion Disk in the Pulsars LMC X-4 and SMC X-1 with NuSTAR and XMM-Newton
Published in The Astrophysical journal (10-01-2020)“…We present a broadband X-ray study of the effect of superorbital periods on X-ray spectra and pulse profiles in the neutron star X-ray binaries LMC X-4 and SMC…”
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5
Going with the Flow: Can the Base of Jets Subsume the Role of Compact Accretion Disk Coronae?
Published in The Astrophysical journal (20-12-2005)“…The hard state of X-ray binaries (XRBs) is characterized by a power-law spectrum in the X-ray band and a flat/inverted radio/IR spectrum associated with…”
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Discovery and modelling of a flattening of the positive cyclotron line/luminosity relation in GX 304−1 with RXTE
Published in Monthly notices of the Royal Astronomical Society (21-04-2017)“…Abstract The Rossi X-ray Timing Explorer (RXTE) observed four outbursts of the accreting X-ray binary transient source, GX 304−1 in 2010 and 2011. We present…”
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GAMMA-RAY OBSERVATIONS OF THE MICROQUASARS CYGNUS X-1, CYGNUS X-3, GRS 1915+105, AND GX 339–4 WITH THE FERMI LARGE AREA TELESCOPE
Published in The Astrophysical journal (01-10-2013)“…Detecting gamma-rays from microquasars is a challenging but worthwhile endeavor for understanding particle acceleration and the jet mechanism and for…”
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NuSTAR DISCOVERY OF A LUMINOSITY DEPENDENT CYCLOTRON LINE ENERGY IN VELA X-1
Published in The Astrophysical journal (10-01-2014)“…We present NuSTAR observations of Vela X-l, a persistent, yet highly variable, neutron star high-mass X-ray binary (HMXB). Two observations were taken at…”
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SPECTRAL AND TIMING NATURE OF THE SYMBIOTIC X-RAY BINARY 4U 1954+319: THE SLOWEST ROTATING NEUTRON STAR IN AN X-RAY BINARY SYSTEM
Published in The Astrophysical journal (10-05-2014)“…The symbiotic X-ray binary (SyXB) 4U 1954+319 is a rare system hosting a peculiar neutron star (NS) and an M-type optical companion. Its ~5.4 hr NS spin period…”
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A Broadband X-Ray View of the Precessing Accretion Disk and Pre-eclipse Dip in the Pulsar Her X-1 with NuSTAR and XMM-Newton
Published in The Astrophysical journal (01-03-2021)“…We present a broad-band X-ray study of the variation with the super orbital cycle of the pulse profiles and spectral shape in the low-mass X-ray binary Her…”
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Accurate Treatment of Comptonization in X-Ray Illuminated Accretion Disks
Published in The Astrophysical journal (01-07-2020)“…A large fraction of accreting black hole and neutron star systems present clear evidence of the reprocessing of X-rays in the atmosphere of an optically thick…”
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A CLUMPY STELLAR WIND AND LUMINOSITY-DEPENDENT CYCLOTRON LINE REVEALED BY THE FIRST SUZAKU OBSERVATION OF THE HIGH-MASS X-RAY BINARY 4U 1538-522
Published in The Astrophysical journal (01-09-2014)“…We present results from the first Suzaku observation of the high-mass X-ray binary 4U 1538-522. The broadband spectral coverage of Suzaku allows for a detailed…”
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INTEGRAL: Science Highlights and Future Prospects
Published in Space science reviews (01-11-2011)“…ESA’s hard X-ray and soft gamma-ray observatory INTEGRAL is covering the 3 keV to 10 MeV energy band, with excellent sensitivity during long and uninterrupted…”
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Evidence for an evolving cyclotron line energy in 4U 1538−522
Published in Monthly notices of the Royal Astronomical Society (21-05-2016)“…We have performed a full time and luminosity-resolved spectral analysis of the high-mass X-ray binary 4U 1538−522 using the available RXTE, INTEGRAL, and…”
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Suzaku Observations of 4U 1957+11: Potentially the Most Rapidly Spinning Black Hole in (the Halo of) the Galaxy
Published in The Astrophysical journal (10-01-2012)“…We present three Suzaku observations of the black hole candidate 4U 1957+11 (V1408 Aql)-a source that exhibits some of the simplest and cleanest examples of…”
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THE Be/X-RAY BINARY SWIFT J1626.6–5156 AS A VARIABLE CYCLOTRON LINE SOURCE
Published in The Astrophysical journal (01-01-2013)“…Swift J1626.6-5156 is a Be/X-ray binary that was in outburst from 2005 December until 2008 November. We have examined Rossi X-ray Timing Explorer/Proportional…”
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Chandra X-Ray Spectroscopy of the Focused Wind in the Cygnus X-1 System. I. The Nondip Spectrum in the Low/Hard State
Published in The Astrophysical journal (01-01-2009)“…We present analyses of a 50 ks observation of the supergiant X-ray binary system Cygnus X-1 (Cyg X-1)/HDE226868 taken with the Chandra High Energy Transmission…”
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CONFIRMATION OF A HIGH MAGNETIC FIELD IN GRO J1008–57
Published in The Astrophysical journal (10-09-2014)“…GRO J1008-57 is a high-mass X-ray binary for which several claims of a cyclotron resonance scattering feature near 80 keV have been reported. We use NuSTAR,…”
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MEASUREMENTS OF CYCLOTRON FEATURES AND PULSE PERIODS IN THE HIGH-MASS X-RAY BINARIES 4U 1538–522 AND 4U 1907+09 WITH THE INTERNATIONAL GAMMA-RAY ASTROPHYSICS LABORATORY
Published in The Astrophysical journal (01-11-2013)“…We present a spectral and timing analysis of International Gamma-Ray Astrophysics Laboratory (INTEGRAL) observations of two high-mass X-ray binaries, 4U…”
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OBSERVATIONS OF THE HIGH-MASS X-RAY BINARY A 0535+26 IN QUIESCENCE
Published in The Astrophysical journal (10-06-2013)“…We have analyzed three observations of the high-mass X-ray binary A 0535+26 performed by the Rossi X-Ray Timing Explorer (RXTE) three, five, and six months…”
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