Do X-ray binary spectral state transition luminosities vary?
A&A, 409 2 (2003) 697-706
Published online: 2003-11-17
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Probing the Disk–Corona Systems and Broad-line Regions of Changing-look Quasars with X-Ray and Optical Observations
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Fainter harder brighter softer: a correlation between αox, X-ray spectral state, and Eddington ratio in tidal disruption events
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The stringent upper limit on jet power in the persistent soft-state source 4U 1957+11
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Kinetic Alfvén Waves in Laboratory, Space, and Astrophysical Plasmas
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Do stellar-mass and super-massive black holes have similar dining habits?
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Accretion Flow Evolution of a New Black Hole Candidate MAXI J1348–630 during the 2019 Outburst
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A radio parallax to the black hole X-ray binary MAXI J1820+070
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Eclipses of jets and discs of X-ray binaries as a powerful tool for understanding jet physics and binary parameters
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The case for jets in cataclysmic variables
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Exploring the Interstellar Medium Using an Asymmetric X-Ray Dust Scattering Halo
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Investigating state transition luminosities of Galactic black hole transients in the outburst decay
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NuSTAR and Chandra Observations of New X-Ray Transients in the Central Parsec of the Galaxy
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Discovery of a transient ultraluminous X-ray source in the elliptical galaxy M86
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The Radio/X-Ray Correlation in X-Ray Binaries—Insights from a Hard X-Ray Perspective
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Late-time UV Observations of Tidal Disruption Flares Reveal Unobscured, Compact Accretion Disks∗
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Hot Accretion Flow around Neutron Stars
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Evolution of X-ray irradiation during the 1999–2000 outburst of the black hole binary XTE J1859 + 226
Mariko Kimura and Chris DoneMonthly Notices of the Royal Astronomical Society 482 (1) 626 (2019)
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