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 2011 · astro-ph.HEShow all

9 papers · 2 filters

astro-ph.HE2011★ 69 cited

The missing link: a low mass X-ray binary in M31 seen as an ultraluminous X-ray source

Matthew J. Middleton, Andrew D. Sutton, Timothy P. Roberts +2

A new, transient ultraluminous X-ray source (ULX) was recently discovered by Chandra in M31 with a luminosity at ~ 5 x 10^39 erg/s. Here we analyse a series of five subsequent XMM-…

astro-ph.HE2011★ 192 cited

A Combined Optical and X-ray Study of Unobscured Type 1 AGN. I. Optical Spectra and SED Modeling

C. Jin, M. Ward, C. Done +1

We present modeling and interpretation of the continuum and emission lines for a sample of 51 unobscured Type 1 active galactic nuclei (AGN). All of these AGNs have high quality sp…

astro-ph.HE2011★ 135 cited

Modelling variability in black hole binaries: linking simulations to observations

Adam Ingram, Chris Done

Black hole accretion flows show rapid X-ray variability. The Power Spectral Density (PSD) of this is typically fit by a phenomenological model of multiple Lorentzians for both the…

astro-ph.HE2011★ 21 cited

Spectral and Timing Studies of Cyg X-1 in the Low/Hard State with Suzaku

Shunsuke Torii, Shin'ya Yamada, Kazuo Makishima +6

From 2005 to 2009, 25 observations of Cyg X-1 were performed with Suzaku, achieving a total exposure of 446 ks. In all observations, the source was found in the low/hard state, whi…

astro-ph.HE2011★ 622 cited

Intrinsic disc emission and the Soft X-ray Excess in AGN

Chris Done, Shane Davis, Chichuan Jin +2

(Abridged) Narrow Line Seyfert 1 (NLS1) galaxies have low mass black holes and mass accretion rates close to (or exceeding) Eddington, so a standard blackbody accretion disc should…

astro-ph.HE2011★ 74 cited

Evidence for a change in the X-ray radiation mechanism in the hard state of Galactic black holes

M. A. Sobolewska, I. E. Papadakis, C. Done +1

We present results on spectral variability of two Galactic black hole X-ray binaries, GRO J1655-40 and GX 339-4, in the hard state. We confirm a transition in behaviour of the phot…

astro-ph.HE2011★ 72 cited

Modelling the high mass accretion rate spectra of GX 339-4: Black hole spin from reflection?

Mari Kolehmainen, Chris Done, Maria Diaz Trigo

We extract all the XMM-Newton EPIC pn burst mode spectra of GX 339-4, together with simultaneous/contemporaneous RXTE data. These include three disc dominated and two soft intermed…

astro-ph.HE2011★ 4 cited

Unlocking the nature of ultraluminous X-ray sources using their X-ray spectra

Jeanette C. Gladstone, Timothy P. Roberts, Chris Done

We explore the nature of ultraluminous X-ray sources through detailed investigations of their spectral shape using some of the highest quality data available in the XMM-Newton publ…

astro-ph.HE2011★ 34 cited

Comparing Spectral Models for ULXs with NGC 4517 ULX1

D. J. Walton, J. C. Gladstone, T. P. Roberts +4

We present the previously unanalysed high quality XMM-Newton spectrum of an ultraluminous X-ray source candidate in NGC 4517. As with other high quality ULX spectra, a downturn in…