The disc instability model of dwarf-novae and low-mass X-ray binary transients

Abstract

The disc instability model which is supposed to describe outbursts of dwarf nova and low-mass X-ray binary transient systems is presented and reviewed in detail. Various deficiencies of the model are pointed out and various remedies and generalizations are presented and discussed.

102 pages, 36 figures (43 postscript files); New Astronomy Reviews, in press

Cited by in corpus (660)

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• The Evolution of Compact Binary Star Systems
• The disc instability model for X-ray transients: evidence for truncation and irradiation
• On the formation and evolution of black-hole binaries
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• Study of Superoutbursts and Superhumps in SU UMa Stars by the Kepler Light Curves of V344 Lyrae and V1504 Cygni
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• Data Mining for Dwarf Novae in SDSS, GALEX and Astrometric Catalogues
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• Mining the Aql X-1 long term X-ray light curve
• X-ray variations in the inner accretion flow of Dwarf Novae
• Population Synthesis of Black Hole X-Ray Binaries
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• The X-ray Properties of M101 ULX-1 = CXOKM101 J140332.74+542102
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• Chandra observations of the neutron star soft X-ray transient RXJ170930.2-263927 returning to quiescence
• Implications of the delayed 2013 outburst of the ESO 243-49 HLX-1
• The long term optical behaviour of helium accreting AM CVn binaries
• Swift Observations of the bright uncatalogued X-ray transient MAXI J1535-571
• Kepler K2 observations of the transitional millisecond pulsar PSR J1023+0038
• Observations of the 599 Hz Accreting X-ray Pulsar IGR J00291+5934 during the 2004 Outburst and in Quiescence
• Nebular emission from young stellar populations including binary stars
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• Random time series in Astronomy
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• Modeling of non-stationary accretion disks in X-ray novae A 0620-00 and GRS 1124-68 during outburst
• Earth, Moon, Sun, and CV Accretion Disks
• MOCCA-SURVEY database I. Accreting white dwarf binary systems in globular clusters -- I. cataclysmic variables -- present-day population
• Delays in dwarf novae: VW Hyi, the tidal instability and enhanced mass transfer models
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• A Synthetic Spectrum and Light Curve Analysis of the Cataclysmic Variable IX Velorum
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• Colours of black holes: infrared flares from the hot accretion disc in XTE J1550-564
• A possible solution of the puzzling variation of the orbital period of MXB 1659-298
• On the X-Ray Light Curve, Pulsed-Radio Emission, and Spin Frequency Evolution of the Transient Anomalous X-Ray Pulsar Xte J1810--197 During its X-Ray Outburst
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• Swift observations of GW Lib: a unique insight into a rare outburst
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• HLX-1 may be an SS433 system
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• Regulation of accretion by its outflow in a symbiotic star: the 2016 outflow fast state of MWC 560
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• On the Common Envelope Efficiency
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• X-ray observations of SU UMa throughout six outbursts
• AstroSat Observation of X-ray Dips and State Transition in the Black Hole Candidate MAXI J1803-298
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• Serendipitous Kepler observations of a background dwarf nova of SU UMa type
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• The discovery of the 528.6 Hz accreting millisecond X-ray pulsar MAXI J1816-195
• An XMM-Newton observation of the nova-like variable UX UMa: spatially and spectrally resolved two-component X-ray emission
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• The case for jets in cataclysmic variables
• VW Hyi: optical spectroscopy and Doppler tomography
• XMM-Newton observation of MV Lyr and the sandwiched model confirmation
• Turbulent and wind-driven accretion in dwarf novae threaded by a large scale magnetic field
• Outbursts of the intermediate-mass black hole HLX-1: a wind instability scenario
• NICER Discovery of Millisecond X-ray Pulsations and an Ultracompact Orbit in IGR J17494-3030
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• Investigating the mass of the intermediate mass black hole candidate HLX-1 with the SLIMBH model
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• Mass transfer variation in the outburst model of dwarf novae and soft X-ray transients
• Delayed Outburst of H 1743--322 in 2003 and relation with its other outbursts
• An accretion disc instability induced by a temperature sensitive $\alpha$ parameter
• A Chandra X-ray observation of the globular cluster Terzan 1
• The complex evolution of the X-ray binary transient MAXI J1807+132 along the decay of its discovery outburst
• Population synthesis on high-mass X-ray binaries: prospects and constraints from the universal X-ray luminosity function
• Effects of Irradiation on the Evolution of Ultra-compact X-ray Binaries
• The unusual 2006 dwarf nova outburst of GK Perseii
• Evolution of finite viscous disks with time-independent viscosity
• X-ray spectral evolution of SAX J1747.0-2853 during outburst activity and confirmation of its transient nature
• Unraveling the foretime of GRS 1915+105 using AstroSat observations: Wide-band spectral and temporal characteristics
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• Optical variability of the accretion disk around the intermediate mass black hole ESO 243-49 HLX-1 during the 2012 outburst
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• Formation of Black Hole Low-Mass X-ray Binaries
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• Formation and Evolution of Galactic Intermediate/Low-Mass X-ray Binaries
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• Formation of Mass-gap Black Holes from Neutron Star X-ray Binaries with Super-Eddington Accretion
• Searching for flickering statistics in T CrB
• Distances of CVs and related objects derived from Gaia Data Release 1
• Continued cooling of the accretion-heated neutron star crust in the X-ray transient IGR J17480-2446 located in the globular cluster Terzan 5
• Physics of accretion flows around compact objects
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• Suzaku Observations of the Dwarf Nova V893 Scorpii: the Discovery of a Partial X-ray Eclipse
• Strongly absorbed quiescent X-ray emission from the X-ray transient XTE J0421+56 (CI Cam) observed with XMM-Newton
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• New possible class of neutron stars: hot and fast non-accreting rotators
• A Chandra observation of the globular cluster Terzan 1: the neutron-star X-ray transient X 1732-304 in quiescence
• Period change of Superhumps in the WZ Sge-Type Dwarf Nova, HV Virginis
• Accretion-disc model spectra for dwarf-nova stars
• FUV Spectroscopy of the Dwarf Novae SS Cygni and WX Hydri in Quiescence
• A re-establishing jet during an X-ray re-brightening of the Be/X-ray binary Swift J0243.6+6124
• Wideband Study of the Brightest Black Hole X-ray Binary 4U 1543-47 in the 2021 Outburst: Signature of Disk-Wind Regulated Accretion
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• Life after eruption - III. Orbital periods of the old novae V365 Car, AR Cir, V972 Oph, HS Pup, V909 Sgr, V373 Sct and CN Vel
• An Extension of the Athena++ Framework for General Equations of State
• Luminosity dependent change of the emission diagram in the X-ray pulsar 4U 1626-67
• Time-Evolved X-ray Irradiation during the 1999$-$2000 Outburst of the Black-Hole Binary XTE J1859+226
• Synthetic Spectrum Constraints on a Model of the Cataclysmic Variable QU Carinae
• The Relationship Between X-ray Luminosity and Duty Cycle for Dwarf Novae and their Specific Frequency in the Inner Galaxy
• The Swift Bulge Survey: optical and near-IR follow-up featuring a likely symbiotic X-ray binary & a focused wind CV
• Can Isolated Single Black Holes Produce X-ray Novae?
• Disc instabilities and nova eruptions in symbiotic systems: RS Ophiuchi and Z Andromedae
• Study of the X-ray pulsar IGR J19294+1816 with NuSTAR: detection of cyclotron line and transition to accretion from the cold disc
• A change in the outburst recurrence time of the Rapid Burster
• WD+RG systems as the progenitors of Type Ia supernovae
• A study of the evolution of the accretion disk of V2051 Oph through two outburst cycles
• XMM-Newton detection of Nova Muscae 1991 in Quiescence
• Discovery of a transient ultraluminous X-ray source in the elliptical galaxy M86
• On the progenitors of millisecond pulsars by the recycling evolutionary channel
• Peculiar disk behaviors of the black hole candidate MAXI J1348-630 in the hard state observed by Insight-HXMT and Swift
• Evidence for high accretion-rates in Weak-Line T Tauri stars?
• Secular changes in the quiescence of WZ Sge: the development of a cavity in the inner disk
• A Comprehensive X-ray Report on AT2019wey
• A decades-long fast-rise-exponential-decay flare in low-luminosity AGN NGC 7213
• Fast stochastic variability study of two SU UMa systems V1504 Cyg and V344 Lyr observed by Kepler satellite
• Study of the long-term evolution of the accretion dynamics of GX 339-4
• Extreme evaporation of planets in hot thermally unstable protoplanetary discs: the case of FU Ori
• Accretion Scenario of MAXI J1820+070 during 2018 Outbursts with Multi-mission Observations
• Mirror eclipses in the cataclysmic variable IP Peg
• X-ray outbursts of ESO 243-49 HLX-1: comparison with Galactic low-mass X-ray binary transients
• BF Eridani: a cataclysmic variable with a massive white dwarf and an evolved secondary
• A 9-Hr CV With One Outburst in 4 Years of Kepler Data
• Nova V5116 Sgr and searching for superhumps in nova remnants
• Dramatic Spectral Evolution of WZ Sagittae during the 2001 Superoutburst
• Selection Effects on the Orbital Period Distribution of Low Mass Black Hole X-ray Binaries
• Hydrodynamic simulations of irradiated secondaries in dwarf novae
• Resolving the mass transfer in the symbiotic recurrent nova T Coronae Borealis
• Modelling rebrightenings, reflares, and echoes in dwarf nova outbursts
• Variability of the inner dead zone edge in 2D radiation hydrodynamic simulations
• First discovery of QPOs in the dwarf nova HS 2325+8205 based on TESS photometry
• The MAVERIC Survey: Variable Jet-Accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters
• Tilt, Warp, and Simultaneous Precessions in Disks
• Common origin for black holes in both high mass X-ray binaries and gravitational-wave sources
• V4140 Sgr: a short period dwarf nova with a peculiar behavior
• Hystereses in dwarf nova outbursts and low-mass X-ray binaries
• Analytical Model of Disk Evaporation and State Transitions in Accreting Black Holes
• Determination of the turbulent parameter in the accretion disks: effects of self-irradiation in 4U 1543-47 during the 2002 outburst
• Dynamical formation of Black Hole Low-Mass X-Ray Binaries in the field - an alternative to common envelope
• Optical Spectroscopic Observations of Cyg X-1=HDE 226868
• Tidal torques, disc radius variations, and instabilities in dwarf novae and soft X-ray transients
• A New Transient Ultraluminous X-ray Source in NGC 7090
• Fast transitions of X-ray variability in the black hole transient GX 339--4: comparison with MAXI J1820+070 and MAXI J1348-630
• Modelling hystereses observed during dwarf-nova outbursts
• TT Arietis: 40 years of photometry
• Novalike Cataclysmic Variables in the Infrared
• Period--luminosity relation for persistent LMXBs in the near-infrared
• An Accurate Determination of the Optical Periodic Modulation in the X-Ray Binary SAX J1808.4-3658
• Chandra HETG line spectroscopy of the Non-magnetic Cataclysmic Variable SS Cyg
• Disk-jet coupling changes as a possible indicator for outbursts from GX 339-4 remaining within the X-ray hard state
• Time-lag between disk and corona radiation leads to hysteresis effect observed in black-hole X-ray binary MAXI J1348-630
• An Illustration of Modeling Cataclysmic Variables: HST, FUSE, SDSS Spectra of SDSSJ080908.39+381406.2
• Further constraints on neutron star crustal properties in the low-mass X-ray binary 1RXS J180408.9$-$342058
• Prototyping non-equilibrium viscous-timescale accretion theory using LMC X-3
• Multi-wavelength observations of the helium dwarf nova KL Dra through its outburst cycle
• A complete X-ray spectral coverage of the 2010 May-June outbursts of Circinus X-1
• The Superoutburst Duration versus Orbital Period Relation for AM CVn stars
• Outbursts in ultracompact X-ray binaries
• The relation between outburst rate and orbital period in low-mass X-ray binary transients
• The disappearance and reformation of the accretion disc during a low state of FO Aquarii
• Paving the way to simultaneous multi-wavelength astronomy
• A Circumbinary Disk Model for the Rapid Orbital Shrinkage in Black Hole Low-Mass X-ray Binaries
• Extreme Quiescent Variability of the Transient Neutron Star Low-mass X-ray Binary EXO 1745-248 in Terzan 5
• The connection between the UV/optical and X-ray emission in the neutron star low-mass X-ray binary Aql X-1
• The peculiar spectral evolution of the new X-ray transient MAXI J0637-430
• Magnetic field transport in compact binaries
• Formation and Evolution of Accreting Compact Objects
• A 2-hr binary period for the black hole transient MAXI J0637-430
• Two new bursting neutron star low-mass X-ray binaries: Swift J185003.2-005627 and Swift J1922.7-1716
• Voracious vortices in cataclysmic variables: II. Evidence for the expansion of accretion disc material beyond the Roche lobe of the accretor in HT Cassiopeia during its 2017 superoutburst
• Observational tests of the picture of disk accretion
• Rapid bursts of magnetically gated accretion in the intermediate polar V1025 Cen
• Nine New Cataclysmic Variable Stars with Negative Superhumps
• Simultaneous multiwavelength observations of V404 Cygni during its 2015 June outburst decay strengthen the case for an extremely energetic jet-base
• Spectral and timing evolution of MAXI J1631-479 during the 2018-19 outburst with NICER
• On fan-shaped cold MHD winds from Keplerian accretion discs
• Multi-wavelength light curve evolution of Swift J1357.2-0933 during its 2011 outburst
• On the curious pulsation properties of the accreting millisecond pulsar IGR J17379-3747
• A misfired outburst in the neutron star X-ray binary Centaurus X-4
• Demonstration of a magnetic Prandtl number disc instability from first principles
• The December 2015 re-brightening of V404 Cyg: Variable absorption from the accretion disc outflow
• Bursting behavior of the Galactic Center faint X-ray transient GRS 1741.9-2853
• Rapid Optical Variations Correlated with X-rays in the 2015 Second Outburst of V404 Cygni (GS 2023$+$338)
• HS 2325+8205 - an ideal laboratory for accretion disk physics
• MAXI and NuSTAR observations of the faint X-ray transient MAXI J1848-015 in the GLIMPSE-C01 Cluster
• The second ULX transient in M31: Chandra, HST and XMM observations, and evidence for an extended corona
• Seven reflares, a mini-outburst and an outburst : High amplitude optical variations in the black hole X-ray binary Swift J1910.2-0546
• The X-ray corona in the black-hole binary GRO J1655--40 from the properties of non-harmonically related quasi-periodic oscillations
• The long-term optical evolution of the black hole candidate MAXI J1659-152
• RS Ophiuchi: Thermonuclear Explosion or Disc Instability?
• Rms-flux relation and fast optical variability simulations of the nova-like system MV Lyr
• Evidence for changes in the radiative efficiency of transient black hole X-ray binaries
• Magnetically-gated accretion model: application to short bursts in the intermediate polar V1223 Sgr
• Accreting neutron stars: heating of the upper layers of the inner crust
• Spiral structures and temperature distribution in the quiescent accretion disc of the cataclysmic binary V2051 Ophiuchi
• SOAR observations of the high-viscosity accretion disc of the dwarf nova V4140 Sagitarii in quiescence and in outburst
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• Simultaneous photometry and echelle-spectroscopy of the dwarf nova BZ Ursae Majoris during the 2005 January Outburst
• The fading of two transient ULXs to below the stellar mass Eddington limit
• A possible overall scenario for the outburst evolution of MAXI J1820+070 revealed by Insight-HXMT
• Two-dimensional simulations of disks in close binaries: Simulating outburst cycles in cataclysmic variables
• The Infrared Counterpart of the X-Ray Nova XTE J1720-318
• QPE or QPO? -- Quasiperiodic Activity in Low-Mass Galaxy Nuclei
• Evolution of negative superhumps, quasi-periodic oscillations and outbursts in the Z Cam-type dwarf nova AH Her
• {\it Insight}-HXMT View of the BHC Swift J1727.8-1613 during its outburst in 2023
• Detection of millihertz quasi-periodic oscillations in the low-mass X-ray binary 4U 1730--22 with NICER
• Long term radio monitoring of the neutron star X-ray binary Swift J1858.6-0814
• A new approach to the GeV flare of PSR B1259-63/LS2883
• A parameter study of the eclipsing CV in the Kepler field, KIS J192748.53+444724.5
• On the recurrence times of neutron star X-ray binary transients and the nature of the Galactic Centre quiescent X-ray binaries
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
• Magnetic Inclination Evolution of Accreting Neutron Stars in Intermediate/Low-Mass X-ray Binaries
• Long-term temperature evolution of neutron stars undergoing episodic accretion outbursts
• DW Cnc: a micronova with a negative superhump and a flickering spin
• Stratified Global MHD Models of Accretion Disks in Semi-Detached Binaries
• Anomalous nature of outbursts of the black hole candidate 4U 1630-472
• Unveiling the nature of compact object in the LMXB MAXI J1957+032 using Swift-XRT
• Refractory Metal Nuggets -- Formation of the First Condensates in the Solar Nebula
• X-ray variability with spectral state transitions in NS-LMXBs observed with MAXI/GSC and Swift/BAT
• On the X-ray Outbursts of Transient Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters
• The 2013 outburst of a transient very faint X-ray binary, 23" from Sgr A*
• Suppression of X-rays during an optical outburst of the helium dwarf nova KL Dra
• On the morphology of outbursts of accreting millisecond X-ray pulsar Aquila X-1
• Introducing the Condor Array Telescope: III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell
• BG Tri an example of a low inclination RW Sex-type novalike
• Accretion Flow Properties of EXO 1846-031 During its Multi-Peaked Outburst After Long Quiescence
• Searching for Compact Object Candidates from LAMOST Time-Domain Survey of Four K2 Plates
• Back to business: SLX 1746--331 after 13 years of silence
• NICER, NuSTAR and Insight-HXMT views to black hole X-ray binary SLX 1746--331
• Properties of the transient X-ray pulsar Swift J1816.7--1613 and its optical companion
• Near-infrared counterparts of three transient very faint neutron star X-ray binaries
• Thermal solutions of strongly magnetized disks and the hysteresis in X-ray binaries
• Accreting neutron stars: composition of the upper layers of the inner crust
• On the Change of the Inner Boundary of an Optically Thick Accretion Disk around White Dwarfs Using the Dwarf Nova SS Cyg as an Example
• Spin evolution of neutron stars in two modes: implication for millisecond pulsars
• Orbital variations and outbursts of the unusual variable star V1129 Centauri
• Physical modeling of viscous disc evolution around magnetized neutron star. Aql X-1 2013 outburst decay
• Sudden End of X-Ray Outbursts around Periastron of Circinus X-1 Observed with MAXI
• The X-ray view of black-hole candidate Swift J1842.5-1124 during its 2008 outburst
• Variable quiescent state for the neutron-star X-ray transient SAX J1750.8-2900: not such a hot neutron star after all?
• Alignment and precession of a black hole misaligned with its accretion disc: Application to Low Mass X-ray Binaries
• Constraining the duty cycle of transient low-mass X-ray binaries through simulations
• Unexpected late-time temperature increase observed in two neutron star crust cooling sources -- XTE~J1701-462 and EXO~0748-676
• Drifts of the marginally stable burning frequency in the X-ray binaries 4U 1608--52 and Aql X--1
• The impact of precession on the observed population of ULXs
• Investigating the nature and properties of MAXI J1810-222 with radio and X-ray observations
• Spectral and Temporal Studies of Swift\,J1658.2--4242 using {\it AstroSat} Observations with {\tt JeTCAF} Model
• PSR J1953+1844 probably being the descendant of an Ultra-compact X-ray binary
• Investigation of superhumps in SU UMa-type dwarf novae based on the observations of TESS
• The bright black hole X-ray binary 4U 1543--47 during 2021 outburst: a thick accretion disk inflated by high luminosity
• The progenitors of Type Ia supernovae with asymptotic giant branch donors
• Optical and Ultraviolet Monitoring of the Black Hole X-ray Binary MAXI J1820+070/ASASSN-18ey for 18 Months
• A Sparkler in the Fireworks Galaxy: Discovery of an Ultraluminous X-ray Transient with a Strong Oxygen Line in NGC 6946
• Solving the Riemann Problem for Realistic Astrophysical Fluids
• Evolution of broad-band SED during outburst rise in NS X-ray Nova Aql X-1
• The Kepler and Hale observations of V523 Lyr
• Common Envelope Mechanisms: Constraints from the X-ray Luminosity Function of High Mass X-ray Binaries
• Photometric Studies of New Southern SU UMa-type dwarf novae, FL Triangulum Australe and CTCV J0549-4921
• Mass accretion rate of the galactic black hole A0620-00 in its quiescent state
• The behaviour of quiescent accretion discs in dwarf novae
• Infrared photometry of the dwarf nova V2051 Ophiuchi: II -- The quiescent accretion disc and its spiral arms
• A search for near-infrared counterparts of two faint neutron star X-ray transients : XMMU J174716.1-281048 and SAX J1806.5-2215
• Suzaku X-Ray Observation of the Dwarf Nova Z Camelopardalis at the Onset of an Optical Outburst
• Insight-HXMT, NICER and NuSTAR views to the newly discovered black hole X-ray binary Swift J151857.0--572147
• A New Window for Studying Intermediate Polars and Tilted Accretion Disk Precession
• Coherent brightness modulations in the dwarf nova AT Cancri
• The Role of Thermal Instability in Accretion Outbursts in High-Mass Stars
• Alternation of the flickering morphology between the high and low state in MV Lyr
• Flickering around the outburst cycle in Kepler dwarf novae
• On the ultra-compact nature of the neutron star system 1RXS J170854.4-321857: insights from X-ray spectroscopy
• Near-ultraviolet detections of four dwarf nova candidates in the globular cluster 47 Tucanae
• Does the accreting millisecond pulsar XTE J1814-338 precess?
• Fourier time lags in the dwarf nova SS Cygni
• Flux Modulation from Non-Axisymmetric Stuctures in Accretion Discs
• A Luminous X-ray Flare From The Nucleus of The Dormant Bulgeless Spiral Galaxy NGC 247
• Evolution of redback radio pulsars in globular clusters
• Relation between the X-ray and Optical Luminosities in Binary Systems with Accreting Nonmagnetic White Dwarfs
• Discovery of a long thermonuclear X-ray burst from the ultra-compact binary 4U 1850$-$087
• Sample of optically unidentified X-ray binaries in the Galactic bulge. Constraints on the physical nature from infrared photometric surveys
• Probing the accretion geometry of the atoll source 4U 1702-429 in different spectral states with NICER, NuSTAR, and AstroSat
• Time lag in transient cosmic accreting sources
• A systematic study of spiral density waves in the accretion discs of Cataclysmic Variables
• OAO/MITSuME Photometry of Dwarf Novae. III. CSS130418:174033+414756
• The statistical significance of the superhump signal in U Gem
• Probing black-hole accretion through time variability
• Magnetohydrodynamic convection in accretion discs
• Evolution of low-mass binaries with black-hole components
• Importance of thermal diffusion in the gravo-magnetic limit cycle
• Tilted Disk Precession and Negative Superhumps in HS 2325+8205: A Multi-Window Analysis
• IGRJ18179-1621: An obscured X-ray pulsar discovered by INTEGRAL
• Optical Spectroscopic Observations of CI Camelopardalis
• The 2015 superoutburst of QZ Virginis: Detection of growing superhumps between the precursor and main superoutburst
• The time step constraint in radiation hydrodynamics
• Evaluating the jet/accretion coupling of Aql X-1: probing the contribution of accretion flow spectral components
• The outbursts properties of AM CVn stars
• Accretion disc winds in X-ray binaries
• Discovery of a new black hole transient within 100" (400 pc) of M31*
• Spectral properties of soft X-ray transient MAXI J0637$-$430 using AstroSat
• A New IW And-Type Star: Karachurin 12 with Tilted Disks and Diverse cycles
• Multiwavelength monitoring of a very active dwarf nova AX J1549.8$-$5416 with an unusually high duty cycle
• Superoutbursts and Positive Superhumps Occurred During the Standstill of a Z Cam-type Dwarf Nova
• Clockwise evolution in the hardness-intensity diagram of the black hole X-ray binary Swift J1910.2-0546
• A Phenomenological Model for the Light Curve of three Quiescent Low-inclination Dwarf Novae and one Pre-Cataclysmic Variable
• AT 2020iko: a WZ Sge-type DN candidate with an anomalous precursor event
• QPOs in compact binaries from small scale eruptions in an inner magnetized disk
• Searching for the 1 mHz variability in the flickering of V4743 Sgr: a Cataclysmic Variable accreting at a high rate
• The origin of UV/optical emission in the black hole low-mass X-ray binary Swift J1753.5-0127
• Swift/XRT, Chandra and XMM-Newton observations of IGR J17091-3624 as it returns into quiescence
• Variation of mass accretion rate onto the white dwarf in the dwarf nova VW Hyi in quiescence
• An approach for solving the boundary free edge difficulties in SPH modelling: application to a viscous accretion disc in close binaries
• MN Draconis - peculiar, active dwarf nova in the period gap
• Turbulent fluctuations and the excitation of Z Cam outbursts
• Millinovae: A New Class of Transient Supersoft X-ray Sources without a Classical Nova Eruption
• Global Disk Oscillation Modes in Cataclysmic Variables and Other Newtonian Accretors
• Modeling the high-brightness state of the recurrent nova T CrB as an enhanced mass-transfer event
• Characterising the short-orbital period X-ray transient Swift J1910.2-0546
• Reverberation lags viewed in hard X-rays from an accreting stellar-mass black hole
• The role of detailed gas and dust opacities in shaping the evolution of the inner disc edge subject to episodic accretion
• The progenitor of binary millisecond radio pulsar PSR J1713+0747 (Research Note)
• Peculiarities of the Accretion Flow in the System HL CMa
• Searching for supergiant fast X-ray transients with Swift
• MITSuME observation of V404 Cygni in the 2015 outburst: Two optical variable components with different variability
• Broad Observational Perspectives Achieved by the Accreting White Dwarf Sciences in the XMM-Newton and Chandra Eras
• Evolution of Accretion Disk Structure of the Black Hole X-ray Binary MAXI J1820$+$070 during the Rebrightening Phase
• The stress-pressure lag in MRI turbulence and its implications for thermal instability in accretion discs
• Effect of Dust Evaporation and Thermal Instability on Temperature Distribution in a Protoplanetary Disk
• Multiwavelength survey of X-ray sources in the Sculptor Dwarf Spheroidal Galaxy
• A Multi-wavelength Characterization of the 2023 Outburst of MAXI J1807+132: Manifestations of Disk Instability and Jet Emission
• Transient behavior of three SU UMa-type dwarf novae; AR Pic, QW Ser and V521 Peg
• Disc-Magnetosphere interactions in Cataclysmic Variable Stars
• Observability of HOFNARs with SRG/eROSITA
• The effect of thermal winds on the outbursts evolution of LMXB systems
• Optical and X-ray variations during 5 outbursts of Aql X-1 in 3.6 years from 2016
• Spectra of accretion discs around white dwarfs
• Quiescent luminosities of transiently accreting neutron stars with neutrino heating due to charged pion decay
• Review: Accretion Disk Evolution in Tidal Disruption Events
• The dependence of the viscosity-parameter on the disk scale height profile
• The hydrogen Balmer lines and jump in absorption in accretion disc modeling -- an ultraviolet-optical spectral analysis of the dwarf novae UZ Serpentis and CY Lyrae
• XMM-Newton observation of V1504 Cyg as a probe for the existence of an evaporated corona
• Typical X-ray Outburst Light Curves of Aql X-1
• A tentative 114-minute orbital period challenges the ultra-compact nature of the X-ray binary 4U 1812-12
• Evolution of the Quiescent Disk surrounding a Superoutburst of the Dwarf Nova TW Virginis
• Accretion Discs with an Inner Spiral Density Wave
• Spiral-wave-driven accretion in quiescent dwarf novæ
• Swift J1753.5-0127 : Understanding the accretion geometry through frequency resolved spectroscopy
• Analysis of accretion disc structure and stability using open code for vertical structure
• Episodic accretion in high-mass star formation: An analysis of thermal instability for axially symmetric disks
• The orbital period and inclination of the neutron star X-ray transient MAXI J1807+132
• Challenging the disk instability model: I -- The case of YZ LMi
• FUSE Observations of the Dwarf Nova SW UMa During Quiescence
• Recurrent outbursts revealed in 3XMM J031820.8-663034
• Photometric analysis of the dwarf nova SU UMa based on TESS
• The youngest of hot jupiters in action: episodic accretion outbursts in Gaia20eae
• Ultraviolet spectroscopy of the black hole X-ray binary MAXI J1820+070 across a state transition
• Influence of inhomogeneous stochasticity on the falsifiability of mean-field theories and examples from accretion disc modeling
• Spectral and Timing Analysis of NuSTAR and Swift/XRT Observations of the X-Ray Transient MAXI J0637-430
• TUVO-21acq: a new cataclysmic variable discovered through a UV outburst
• The X-ray binaries in M83: will any of them form gravitational wave sources for LIGO/VIRGO/KAGRA?
• Mass-transfer Outburts reborn: Modeling the light curve of the dwarf nova EX Draconis
• Searching for similarities in the accretion flow of Seyfert 1 galaxies and cataclysmic variables based on flare profiles of IRAS 13224-3809, 1H 0707-495, Mrk 766 and MV Lyr
• The peculiar disk evolution of 4U 1630--472 observed by Insight-HXMT during the 2022 and 2023 outbursts
• V1047 Cen: The first Z And-type outburst observed in the classical nova binary
• A MeerKAT survey of nearby dwarf novae: I. New detections
• Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility
• The NuSTAR view of Ultra-Compact X-ray Binaries
• Accretion Geometry of Black Hole X-ray Binaries: Insights from X-ray Observations
• Fundamental Parameters of Low Mass X-ray Binaries II: X-Ray Persistent Systems
• An X-ray and Optical Study of the Dwarf Nova Candidate OGLE-BLG-DN-0064
• A large population of neutron star low-mass X-ray binaries with long outburst recurrence time ?
• OGLE-BLG504.12.201843: A possible extreme dwarf nova
• Long-term photometric behavior of the eclipsing cataclysmic variable V729 Sgr
• Infrared photometry of the dwarf nova V2051 Ophiuchi: I - The mass donor star and the distance
• On Pulsar-Driven Mass Ejection in Low-Mass X-ray Binaries
• Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
• X-ray and UV correlation in the quiescent emission of Cen X-4, evidence of accretion and reprocessing
• Galactic X-ray Transients in the First eROSITA All Sky Survey
• Ultraluminous X-ray sources in the first eROSITA survey I. Candidate catalogs
• SMSS J130522.47-293113.0: a high-latitude stellar X-ray source with pc-scale outflow relics?
• Long thermonuclear burst driven thermal-viscous instability of accretion disk: triggering an outburst-like X-ray flare
• Resolving SLX 1744-299 and SLX 1744-300 in the hard X-ray band: implications for their ultracompact nature
• Observational Biases and Improved Modelling of Off-axis Relativistic Jets
• An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise
• A candidate to the long sought optical counterpart to the Rapid Burster in the bulge fossil fragment Liller 1
• Fast giant flares in discs around supermassive black holes
• Chandra, XMM-Newton and HST observations of a transient in M31 with a possible asymmetric, precessing disk
• Discovery of a probable very fast extragalactic nova in a symbiotic binary
• Time Domain Astronomy with the THESEUS Satellite
• Swift observations of the dwarf nova ASASSN-18fs
• Probing the accretion disk - jet connection via instabilities in the inner accretion flow. From microquasars to quasars
• Photospheric Radius Expansion and a double-peaked type-I X-ray burst from GRS 1741.9-2853
• White Dwarf Mass Growth in Cataclysmic Variables: Roles of Dwarf Novae
• Evolution of X-ray and optical rapid variability during the low/hard state in the 2018 outburst of MAXI J1820+070 = ASASSN-18ey