activity
19952026
most citedModelling the behaviour of accretion flows in X-ray binaries

1.3k citations · 17.2k across the 252 of their papers we have counts for

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Showing 2018 · astro-ph.HEShow all

12 papers · 2 filters

astro-ph.HE2018★ 195 cited

The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey

R. Edelson, J. Gelbord, E. Cackett +32

Swift intensive accretion disk reverberation mapping of four AGN yielded light curves sampled 200-350 times in 0.3-10 keV X-ray and six UV/optical bands. Uniform reduction an…

astro-ph.HE2018★ 61 cited

Reverberation Reveals the Truncated Disc in the Hard State of GX 339-4

Ra'ad D. Mahmoud, Chris Done, Barbara De Marco

The nature and geometry of the hard state in black hole binaries is controversial. The broadband continuum spectrum and fast variability properties can be explained in a model wher…

astro-ph.HE2018★ 58 cited

Line-driven disc wind in near-Eddington active galactic nuclei: decrease of mass accretion rate due to powerful outflow

Mariko Nomura, Ken Ohsuga, Chris Done

Based on recent X-ray observations, ultra-fast outflows from supermassive black holes are expected to have enough energy to dramatically affect their host galaxy but their launch a…

astro-ph.HE2018★ 39 cited

Detection of polarized gamma-ray emission from the Crab nebula with Hitomi Soft Gamma-ray Detector

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +191

We present the results from the Hitomi Soft Gamma-ray Detector (SGD) observation of the Crab nebula. The main part of SGD is a Compton camera, which in addition to being a spectrom…

astro-ph.HE2018★ 25 cited

X-ray reverberation lags of the Fe-K line due to AGN disc winds

Misaki Mizumoto, Ken Ebisawa, Masahiro Tsujimoto +3

Short X-ray reverberation lags are seen across a broad Fe-K energy band in more than twenty active galactic nuclei (AGNs). This broad iron line feature in the lag spectrum is most…

astro-ph.HE2018★ 19 cited

Time-Evolved X-ray Irradiation during the 19992000 Outburst of the Black-Hole Binary XTE J1859+226

Mariko Kimura, Chris Done

X-ray irradiation in X-ray binaries is thought to control the behavior at the outer disc, which is observable mainly at optical wavelengths. It is generally parameterized phenomeno…

astro-ph.HE2018★ 26 cited

X-ray short-time lags in the Fe-K energy band produced by scattering clouds in active galactic nuclei

Misaki Mizumoto, Chris Done, Kouichi Hagino +3

X-rays illuminating the accretion disc in active galactic nuclei give rise to an iron K line and its associated reflection spectrum which are lagged behind the continuum variabilit…

astro-ph.HE2018★ 253 cited

A physical model of the broadband continuum of AGN and its implications for the UV/X relation and optical variability

Aya Kubota, Chris Done

We develop a new spectral model for the broadband spectral energy distribution (SED) of Active Galactic Nuclei (AGN). This includes an outer standard disc, an inner warm Comptonisi…

astro-ph.HE2018★ 27 cited

Breaking the spectral degeneracies in black hole binaries with fast timing data

M. Axelsson, C. Done

The spectra of black hole binaries in the low/hard state are complex, with evidence for multiple different Comptonisation regions contributing to the hard X-rays in addition to a c…

astro-ph.HE2018★ 47 cited

A Physical Model for the Spectral-Timing Properties of Accreting Black Holes

Ra'ad D. Mahmoud, Chris Done

We develop new techniques to deconvolve the radial structure of the X-ray emission region in the bright low/hard state of the black hole Cygnus X-1 using both spectral and timing d…

astro-ph.HE2018★ 17 cited

Monte-Carlo simulations of the detailed iron absorption line profiles from thermal winds in X-ray binaries

Ryota Tomaru, Chris Done, Hirokazu Odaka +2

Blue shifted absorption lines from highly ionised iron are seen in some high inclination X-ray binary systems, indicating the presence of an equatorial disc wind. This launch mecha…

astro-ph.HE2018★ 16 cited

Hitomi X-ray Observation of the Pulsar Wind Nebula G21.50.9

Hitomi Collaboration, Felix Aharonian, Hiroki Akamatsu +194

We present results from the Hitomi X-ray observation of a young composite-type supernova remnant (SNR) G21.50.9, whose emission is dominated by the pulsar wind nebula (PWN) cont…