Ultraluminous X-ray sources
arXiv:2302.10605 · doi:10.1016/j.newar.2022.101672
Abstract
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 wavebands, and across multiple scales in space and time. We discuss recent progress and current unanswered questions. We consider the range of current theories of ULX properties in the light of this observational progress. Applying these models to neutron-star ULXs offers particularly stringent tests, as this is the unique case where the mass of the accretor is effectively fixed.
arXiv commentA preprint as close as possible to the open access article at: https://www.sciencedirect.com/science/article/pii/S1387647322000306?via%3Dihub
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- Pulsing and Non-Pulsing ULXs: the Iceberg Emerges
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- NGC 300 ULX1: A test case for accretion torque theory
- Revisiting the ultraluminous supersoft source in M101: an optically thick outflow model
- A long-term X-ray monitoring of the ultraluminous X-ray source NGC 5408 X-1 with Swift reveals the presence of dips but no orbital period
- A Super-Eddington Compton-Thick Wind in GRO J1655-40?
- A new globular cluster black hole in NGC 4472
- All at once: transient pulsations, spin down and a glitch from the Pulsating Ultraluminous X-ray Source M82 X-2
- The Lense-Thirring timing-accretion plane for ULXs
- Time lags in the ultraluminous X-ray source NGC 5408 X-1: implications for the black hole mass
- Large Highly-Ionized Nebulae Around Ultra-luminous X-ray Sources
- Chandra monitoring observations of the ultraluminous X-ray source NGC 5204 X-1
- The observed vs total population of ULXs
- The slimming effect of advection on black-hole accretion flows
- Thermal stability of winds driven by radiation pressure in super-Eddington accretion disks
- Low density, radiatively inefficient rotating-accretion flow onto a black hole
- Nature of the Extreme Ultraluminous X-ray Sources
- Implications of the delayed 2013 outburst of the ESO 243-49 HLX-1
- A Radio Monitoring Survey of Ultra-Luminous X-Ray Sources
- A Luminous Recurrent Supersoft X-ray Source in NGC 300
- General relativistic radiation magnetohydrodynamics simulations of supercritical accretion onto magnetized neutron star; -modeling of ultra luminous x-ray pulsars
- Anti-glitches in the Ultraluminous Accreting Pulsar NGC 300 ULX-1 Observed with NICER
- Evidence for precession due to supercritical accretion in ultraluminous X-ray sources
- Detection of Strong Short-Term Variability in NGC 6946 X-1
- Wind Roche Lobe Overflow as a way to make type Ia supernova from the widest symbiotic systems
- Supercritical Accretion onto a Non-Magnetized Neutron Star: Why is it Feasible?
- Swift monitoring of M51: A 38-day super-orbital period for the pulsar ULX7 and a new transient ULX
- Evidences of the supercritical disc funnel radiation in X-ray spectra of SS 433
- Extremely fast orbital decay of the black hole X-ray binary Nova Muscae 1991
- Long-term evolution of supercritical black hole accretion with outflows: a subgrid feedback model for cosmological simulations
- Modeling the light curves of ultraluminous X-ray sources as precession
- The First Detection of [O IV] from an Ultraluminous X-ray Source with Spitzer. II. Evidence for High Luminosity in Holmberg II ULX
- The Orbital Period of the Ultraluminous X-ray Source in M82
- Milliarcsec-scale radio emission of ultraluminous X-ray sources: steady jet emission from an intermediate-mass black hole?
- Chandra reveals a possible ultra-fast outflow in the super-Eddington Be/X-ray binary Swift J0243.6+6124
- The Hunt for Pulsating Ultraluminous X-ray Sources
- Direct Detection of an Ultraluminous Ultraviolet Source
- Radiation hydrodynamics simulations of wide-angle outflows from super-critical accretion disks around black holes
- Evidence for High-Frequency QPOs with a 3:2 Frequency Ratio from a 5000 Solar Mass Black Hole
- Irradiated, colour-temperature-corrected accretion discs in ultraluminous X-ray sources
- A Multi-epoch Timing and Spectral Study of the Ultraluminous X-Ray Source NGC 5408 X-1 with XMM-Newton
- Three new X-ray pulsars detected in the Small Magellanic Cloud and the positions of two other known pulsars determined
- Searching for Massive Outflows in Holmberg IX X-1 and NGC 1313 X-1: The Iron K Band
- Accretion torque on magnetized neutron stars
- The Broadband Spectral Variability of Holmberg IX X-1
- Investigating ULX accretion flows and cyclotron resonance in NGC 300 ULX1
- Science with the X-ray Imaging and Spectroscopy Mission (XRISM)
- X-ray time lags and nonlinear variability in the ultraluminous X-ray sources NGC 5408 X-1 and NGC 6946 X-1
- Thermally-Driven Disc Winds as a Mechanism for X-ray Irradiation Heating in Black Hole X-ray Binaries: The Case Study of GX339-4
- Two eclipsing ultraluminous X-ray sources in M 51
- Slim accretion disks around black holes
- Discovery of a Glitch in the Accretion Powered Pulsar SXP 1062
- Chandra ACIS Survey of X-ray Point Sources in Nearby Galaxies. II. X-ray Luminosity Functions and Ultraluminous X-ray Sources
- Ultra-luminous X-ray Sources as Supercritical Accretion Disks: Spectral Energy Distributions
- Orbital and super-orbital periods in ULX pulsars, disc-fed HMXBs, Be/X-ray binaries and double-periodic variables
- X-Ray Spectral Variability of Ultraluminous X-Ray Sources in Extragalactic Globular Clusters
- Large-scale outflow structure and radiation properties of super-Eddington flow: Dependence on the accretion rates
- The Physical Parameters of the Micro-quasar S26 in the Sculptor Group Galaxy NGC 7793
- MUSE spectroscopy of the ULX NGC 1313 X-1: a shock-ionised bubble, an X-ray photoionised nebula, and two supernova remnants
- Evidence for Optically Thick, Eddington-limited Winds Driven by Supercritical Accretion
- Super-Eddington Emission from Accreting, Highly Magnetised Neutron Stars with a Multipolar Magnetic Field
- Uncovering Red and Dusty Ultraluminous X-ray Sources with Spitzer
- SWIFT Detection of a 65-Day X-ray Period from the Ultraluminous Pulsar NGC 7793 P13
- The connection between merging double compact objects and the Ultraluminous X-ray Sources
- NIR Counterparts to ULXs (III): Completing the photometric survey and selected spectroscopic results
- A deficit of ultraluminous X-ray sources in luminous infrared galaxies
- The Jets and Disc of SS 433 at Super-Eddington Luminosities
- Compact radio emission in Ultraluminous X-ray sources
- Optical counterpart to Swift J0243.6+6124
- X-ray Transients: Hyper- or Hypo-Luminous?
- No Strong Geometric Beaming in the Ultraluminous Neutron Star Binary NGC 300 ULX-1 (SN 2010da) from Swift and Gemini
- The First Detection of [O IV] from an Ultraluminous X-ray Source with Spitzer I. Observational Results for Holmberg II ULX
- On the Magnetic Fields, Beaming Fractions, and Fastness Parameters of Pulsating Ultra-Luminous X-Ray Sources
- The ultraluminous X-ray source bubble in NGC 5585
- Radiative GRMHD simulations of accretion and outflow in non-magnetized neutron stars and ultraluminous X-ray sources
- Ultraluminous X-ray sources with flat-topped noise and QPO
- Discovery of a soft X-ray lag in the Ultraluminous X-ray Source NGC 1313 X-1
- Accreting strongly magnetised neutron stars: X-ray Pulsars
- Optical Spectroscopy of the environment of a ULX in NGC 7331
- Quasi-periodic dipping in the ultraluminous X-ray source, NGC 247 ULX-1
- A Systematic Search for Near-Infrared Counterparts of Nearby Ultraluminous X-ray sources (II)
- Chandra and XMM-Newton discovery of the transient X-ray pulsar in the nearby spiral galaxy NGC2403
- Discovery of a Quasi-Periodic Oscillation in the Ultraluminous X-ray Source IC 342 X-1: XMM-Newton Results
- The effect of advection at luminosities close to Eddington: The ULX in M31
- Searching for the Donor Stars of ULX Pulsars
- A variable ultraluminous X-ray source in a globular cluster in NGC 4649
- Spitzer Observations of MF 16 Nebula and the associated Ultraluminous X-ray Source
- XMM-Newton discovery of transient X-ray pulsar in NGC 1313
- Searching for coherent pulsations in ultraluminous X-ray sources
- Can the 62 day X-ray period of the Ultraluminous X-ray source M82 X-1 be due to a precessing accretion disk?
- Discovery of a Highly Variable Dipping Ultraluminous X-ray source in M94
- Continuous monitoring of pulse period variations in Her X-1 using Swift/BAT
- Towards a dynamical mass of the ultraluminous X-ray source NGC 5408 X-1
- Models of Ultra-Luminous X-ray transient sources
- X-Ray Spectroscopy of Newly Identified ULXs Associated With M87's Globular Cluster Population
- Spectral variability in Swift and Chandra observations of the Ultraluminous source NGC 55 ULX1
- Thermally driven winds in ULXs
- A Possible 55-day X-ray Period of the Ultraluminous Accreting Pulsar M82 X-2
- The (re)appearance of NGC 925 ULX-3, a new transient ULX
- Spectral evolution of the ultraluminous X-ray sources M82 X-1 and X-2
- Size distribution of supernova remnants and the interstellar medium: the case of M33
- Linking soft excess in ultraluminous X-ray sources with optically thick wind driven by supercritical accretion
- The rare X-ray flaring activity of the Ultraluminous X-ray source NGC 4559 X7
- Three Ultraluminous X-ray Sources Hosted by Globular Clusters in NGC 1316
- Eccentricity of HLX-1
- A Wind-Disk Self-Irradiation Model For Supercritical Accretion
- Composition of an Emission Line System in Black Hole Host Globular Cluster RZ2109
- Pulsed fraction of super-critical column accretion flows onto neutron stars: modeling of ultraluminous X-ray pulsars
- Ultraluminous X-ray sources out to z~0.3 in the COSMOS field
- Population synthesis of ultraluminous X-ray sources with magnetised neutron stars
- New observations of ULX supershells, and their implications
- The ionizing and heating power of ultraluminous X-ray sources under the geometrical beaming model
- ULX pulsar Swift J0243.6+6124 observations with NuSTAR -- dominance of reflected emission in the super-Eddington state
- Geometrical beaming of stellar mass ULXs
- Optical Spectroscopy of the ULX-Associated Nebula MF16
- The Binary Black Hole Merger Rate from Ultraluminous X-ray Source Progenitors
- Limits on thickness and efficiency of Polish doughnuts in application to the ULX sources
- A multi-wavelength view of distinct accretion regimes in the pulsating ultraluminous X-ray source NGC 1313 X-2
- Be star discs: powered by a non-zero central torque
- Supermassive Black Hole Demographics: Evading
- Spitzer IRAC observations of IR excess in Holmberg IX X-1: A circumbinary disk or a variable jet?
- Exploring X-ray Binary Populations in Compact Group Galaxies with
- A New Microquasar Candidate in M83
- A disrupted bulgeless satellite galaxy as counterpart of the ultraluminous X-ray source ESO 243-49 HLX-1
- The impact of precession on the observed population of ULXs
- The Brightest Cluster X-ray Sources
- Meta-analysis of Electron Cyclotron Resonance Absorption Features Detected in High-Mass X-ray Binaries
- eROSITA on SRG: a X-ray all-sky survey mission
- Discovery of two eclipsing X-ray binaries in M51
- Disappearing Pulses in Vela X-1
- Evidence for Fe K line and soft X-ray lag in NGC 7456 ULX-1
- Observational limits on the X-ray emission from the bubble nebula surrounding Ho IX X-1
- A search for radio counterparts to Chandra ULX candidates
- One for the Future: measuring the mass transfer rate in the ULX M82 X-2 by using orbital period changes will take millenia
- The Ultraluminous X-ray Source in Holmberg IX and its Environment
- Monitoring and Discovering X-ray Pulsars in the Small Magellanic Cloud
- The Collimated Radiation in SS 433. Constraints from Spatially Resolved Optical Jets and Modeling of the Optical Bullets
Cited by in corpus (56)
- Science objectives of the Einstein Probe mission
- Cygnus X-3 revealed as a Galactic ultraluminous X-ray source by IXPE
- Unequal-mass, highly-spinning binary black hole mergers in the stable mass transfer formation channel
- Search for directional associations between Baikal Gigaton Volume Detector neutrino-induced cascades and high-energy astrophysical sources
- Ultraluminous X-ray sources are beamed
- Particle acceleration and multi-messenger radiation from Ultra-Luminous X-ray Sources: A new class of Galactic PeVatrons
- Dynamical Effects of Magnetic Opacity in Neutron Star Accretion Columns
- Studying geometry of the ultraluminous X-ray pulsar Swift J0243.6+6124 using X-ray and optical polarimetry
- A new sample of transient ultraluminous X-ray sources serendipitously discovered by Swift/XRT
- A new pulsating neutron star in the Ultraluminous X-ray source NGC 4559 X7?
- Getting More Out of Black Hole Superradiance: a Statistically Rigorous Approach to Ultralight Boson Constraints from Black Hole Spin Measurements
- Populations of Neutron Star Ultraluminous X-ray Sources: Mind your b's and B's
- BH-BH mergers with & without EM counterpart: A model for stable tertiary mass transfer in hierarchical triple systems
- X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries
- On the nature of the ultraluminous X-ray source Holmberg II X-1
- GR-RMHD Simulations of Super-Eddington Accretion Flows onto a Neutron Star with Dipole and Quadrupole Magnetic Fields
- Simultaneous NICER and NuSTAR observations of the Ultraluminous source NGC 4190 ULX-1
- The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources
- The Orbit of NGC 5907 ULX-1
- X-ray emission from helium star+black hole binaries as probes of tidally induced spin-up of second-born black holes
- Evidence for Low Universal Equilibrium Black Hole Spin in Luminous Magnetically Arrested Disks
- The innermost jet in the hidden ultra-luminous X-ray source Cygnus X-3
- Constraining the evolution of the unstable accretion disk in SMC X-1 with NICER
- Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor
- SN 2022jli: The ultraluminous birth of a low-mass X-ray binary
- New Transient ULX Candidate in NGC 4254: Evidence of Circumbinary Disk?
- A NuSTAR study of quasi-periodic oscillations from the ultraluminous X-ray sources in M82
- NGC 2403 XMM4: evidence for a super-Eddington neutron star with a possible transient pulsation
- Long-Term X-Ray/UV Variability in ULXs
- Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation
- Searching for the highest energy of pulsation and critical luminosity of Swift J0243.6+6124 observed by Insight-HXMT
- Tilted Accretion Disks
- Spectral analysis of ultraluminous X-ray pulsars with models of X-ray pulsars
- The hunt for new pulsating ultraluminous X-ray sources: a clustering approach
- Ultraluminous X-ray sources in Globular Clusters
- The restless population of bright X-ray sources of NCG 3621
- XMM-Newton multi-year campaign on NGC 55 ULX-1: Resolving the wind and its variability with RGS
- The significant contribution of supersoft X-ray Sources to the nebular HeII line emission
- Phase-Dependent Spectral Shape Changes in the Ultraluminous X-Ray Pulsar NGC 5907 ULX1
- The X-ray Point Source Population Hosted by Globular Clusters in the Elliptical Galaxy NGC 4261
- The population of hyperluminous X-ray sources as seen by XMM-Newton
- A Study of Spectral Variability between flaring and non-flaring state in M74 X-1
- Spectral study of X-ray sources in some galaxies recently observed by Chandra
- The First Glimpse of ULXs Through the Near-Infrared Images Captured by the James Webb Space Telescope
- Identification of three new ultraluminous X-ray sources in NGC 4631 and NGC 1097: Evidence for stellar-mass black holes
- Comprehensive X-ray and Multiwavelength Study of ULXs in NGC 1566
- Optical flares due to X-ray irradiation during BeXRB major outbursts
- Unveiling the biconical geometry of the outflow in the ultraluminous X-ray source NGC 5204 X-1
- Surface gravity wave on a neutron star ocean trapped around a magnetic pole
- Probing spectral variability in NGC 4490 ULX-8 over 24 years of XMM-Newton, Chandra and Swift-XRT observations
- A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
- A Synthetic Population of Ultra-Luminous X-ray Sources: Optical-X-ray Correlation
- Probing extreme black-hole outflows on short timescales via high spectral-resolution X-ray imagers
- The core starbursts of the galaxy NGC 3628: Radio very long baseline interferometry and X-ray studies
- Ultraluminous X-ray sources in the group-centric elliptical galaxy NGC 5813
- Ultraluminous X-ray sources in the first eROSITA survey I. Candidate catalogs