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Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2014, Volume 565, pp. A1 - np
We present the most extensive analysis of Fourier-based X-ray timing properties of the black hole binary Cygnus X-1 to date, based on 12 years of bi-weekly monitoring with RXTE from 1999 to 2011... 
X-rays: binaries | Stars: individual: Cygnus X-1 | Binaries: close | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Power spectra | X-rays | Coherence | Spectra | Time measurements | Astronomy | Monitoring | Time lag | Physics - High Energy Astrophysical Phenomena | Physics | Astrophysics
Journal Article
The Astrophysical journal, ISSN 1538-4357, 12/2011, Volume 742, Issue 2, p. 83
We report a direct and accurate measurement of the distance to the X-ray binary Cygnus X-1, which contains the first black hole to be discovered. The distance of 1.86(-0.11)(+0.12... 
black hole physics | X-rays: binaries | stars: individual (Cygnus X-1) | astrometry | stars: distances | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - High Energy Astrophysical Phenomena | ROTATION | X RADIATION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | DOPPLER EFFECT | ORBITS | PROPER MOTION | STARS | THREE-DIMENSIONAL CALCULATIONS | BLACK HOLES
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 2013, Volume 554, pp. A88 - np
We present a scheme for determining the spectral state of the canonical black hole Cyg X-1 using data from previous and current X-ray all sky monitors... 
X-rays: binaries | Stars: individual: Cygnus X-1 | Binaries: close | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Sky | Phases | Statistical analysis | X-rays | Monitors | Spectra | Time measurements | Astronomy | Physics - High Energy Astrophysical Phenomena
Journal Article
The Astrophysical journal, ISSN 1538-4357, 12/2011, Volume 742, Issue 2, p. 84
Journal Article
Journal Article
The Astrophysical journal, ISSN 1538-4357, 07/2016, Volume 826, Issue 1, pp. 87 - 87
We present a multi-epoch hard X-ray analysis of Cygnus X-1 in its soft state based on four observations with the Nuclear Spectroscopic Telescope Array (NuSTAR... 
X-rays: Binaries | X-rays: Individual (Cygnus X-1) | Black hole physics | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Absorption | Misalignment | Continuums | Mathematical models | Reflection | Spectra | Iron | Accretion disks | Physics - High Energy Astrophysical Phenomena
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 12/2016, Volume 596, p. A55
Aims. We probe the high-energy (>60 MeV) emission from the black hole X-ray binary system, Cygnus X-1, and investigate its origin. Methods. We analyzed... 
Radiation mechanisms: non-thermal | Gamma rays: general | Stars: individual: Cygnus X-1 | X-rays: binaries | Acceleration of particles | Accretion, accretion disks | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Gamma rays | Forats negres (Astronomia) | Raigs gamma | Black holes (Astronomy)
Journal Article