[HTML][HTML] Ultraluminous X-ray sources
The study of ultraluminous X-ray sources (ULXs) has changed dramatically over the last
decade. In this review we first describe the most important observations of ULXs in various …
decade. In this review we first describe the most important observations of ULXs in various …
X-ray properties of black-hole binaries
RA Remillard, JE McClintock - Annu. Rev. Astron. Astrophys., 2006 - annualreviews.org
We review the properties and behavior of 20 X-ray binaries that contain a dynamically-
confirmed black hole, 17 of which are transient systems. During the past decade, many of …
confirmed black hole, 17 of which are transient systems. During the past decade, many of …
WATCHDOG: a comprehensive all-sky database of galactic black hole X-ray binaries
BE Tetarenko, GR Sivakoff, CO Heinke… - The Astrophysical …, 2016 - iopscience.iop.org
With the advent of more sensitive all-sky instruments, the transient universe is being probed
in greater depth than ever before. Taking advantage of available resources, we have …
in greater depth than ever before. Taking advantage of available resources, we have …
The evolution of cataclysmic variables as revealed by their donor stars
C Knigge, I Baraffe, J Patterson - The Astrophysical Journal …, 2011 - iopscience.iop.org
We present an attempt to reconstruct the complete evolutionary path followed by cataclysmic
variables (CVs), based on the observed mass–radius relationship of their donor stars. Along …
variables (CVs), based on the observed mass–radius relationship of their donor stars. Along …
Modelling the behaviour of accretion flows in X-ray binaries: Everything you always wanted to know about accretion but were afraid to ask
C Done, M Gierliński, A Kubota - The Astronomy and Astrophysics Review, 2007 - Springer
We review how the recent increase in X-ray and radio data from black hole and neutron star
binaries can be merged together with theoretical advances to give a coherent picture of the …
binaries can be merged together with theoretical advances to give a coherent picture of the …
X-ray emissions from accreting white dwarfs: a review
K Mukai - Publications of the Astronomical Society of the Pacific, 2017 - iopscience.iop.org
Interacting binaries in which a white dwarf accretes material from a companion—cataclysmic
variables (CVs) in which the mass donor is a Roche-lobe filling star on or near the main …
variables (CVs) in which the mass donor is a Roche-lobe filling star on or near the main …
Explaining changing-look AGN with state transition triggered by rapid mass accretion rate drop
We model the broad-band (optical/UV and X-ray) continuum spectrum of the 'changing-
look'active galactic nucleus (AGN) Mrk 1018, as it fades from Seyfert 1 to 1.9 in∼ 8 years …
look'active galactic nucleus (AGN) Mrk 1018, as it fades from Seyfert 1 to 1.9 in∼ 8 years …
A review of the disc instability model for dwarf novae, soft X-ray transients and related objects
JM Hameury - Advances in Space Research, 2020 - Elsevier
I review the basics of the disc instability model (DIM) for dwarf novae and soft-X-ray
transients and its most recent developments, as well as the current limitations of the model …
transients and its most recent developments, as well as the current limitations of the model …
Black hole binaries
JE McClintock, RA Remillard - arXiv preprint astro-ph/0306213, 2003 - arxiv.org
We review the properties of 40 X-ray binaries that contain either a confirmed black hole or a
black hole candidate. After discussing briefly the significance of these Galactic black holes to …
black hole candidate. After discussing briefly the significance of these Galactic black holes to …
Accretion disc viscosity: how big is alpha?
AR King, JE Pringle, M Livio - Monthly Notices of the Royal …, 2007 - academic.oup.com
We consider observational and theoretical estimates of the accretion disc viscosity
parameter α. We find that in thin, fully ionized discs, the best observational evidence …
parameter α. We find that in thin, fully ionized discs, the best observational evidence …