1.3k citations · 17.2k across the 252 of their papers we have counts for
7 papers · 1 filter
Bright radio emission from an ultraluminous stellar-mass microquasar in M31
Matthew J. Middleton, James C. A. Miller-Jones, Sera Markoff +34
A subset of ultraluminous X-ray sources (those with luminosities < 10^40 erg/s) are thought to be powered by the accretion of gas onto black holes with masses of ~5-20 M_solar, pro…
The effect of frame dragging on the iron K alpha line in X-ray binaries
Adam Ingram, Chris Done
The clear characteristic timescale picked out by the low frequency quasi-periodic oscillations (QPOs) seen in many black hole and neutron star binaries has the potential to provide…
The effect of advection at luminosities close to Eddington: The ULX in M31
Odele Straub, Chris Done, Matthew J. Middleton
The transient, ultra-luminous X-ray source CXOM31 J004253.1+411422 in the Andromeda galaxy is most likely a 10 solar mass black hole, with super-Eddington luminosity at its peak. T…
Jets and the Accretion Flow in Low Luminosity Black Holes
Emma Gardner, Chris Done
The X-ray spectra of black hole binaries in the low/hard state first harden as the flux decreases, then soften. This change in behaviour has been variously attributed to either the…
A combined Optical and X-ray Spectra Study for Type 1 AGN. III. Broadband SED Properties
Chichuan Jin, Martin Ward, Chris Done
In this third paper in a series of three, we present a detailed study of the AGN broadband SED based on a nearby unobscured Type 1 AGN sample. We perform a systematic cross-correla…
The truncated disk from Suzaku data of GX 339-4 in the extreme very high state
Manami Tamura, Aya Kubota, Shinya Yamada +4
We report on the geometry of accretion disk and high energy coronae in the strong Comptonization state (the very high/steep power law/hard intermediate state) based on a Suzaku obs…