ADAFs, accretion discs and outbursts in compact binaries
arXiv:0801.0490 · doi:10.1016/j.newar.2008.03.003
Abstract
I discuss the status of the Soft X-ray Transient model. First, I discuss and then compare with observations the assumption that the geometrically thin disc evaporates into an ADAF. Second, I address the problems created by the recent determinations of the distance to SS Cyg, according to which the Disc Instability Model does not apply to this famous dwarf-nova, thus casting doubt on the application of this model to any system at all.
To be published in New Astronomy Review (Proceedings of the meeting "JPL, X-ray binaries, accretion disks and compact stars", October 2007, Editor: M.A. Abramowicz), Eq. (2) corrected
References in corpus (35)
- On the Fate of Gas Accreting at a Low Rate onto a Black Hole
- Advection-Dominated Accretion and the Spectral States of Black Hole X-Ray Binaries: Application to Nova Muscae 1991
- The disc instability model of dwarf-novae and low-mass X-ray binary transients
- Crustal Heating and Quiescent Emission from Transiently Accreting Neutron Stars
- The disc instability model for X-ray transients: evidence for truncation and irradiation
- A New Model for Black Hole Soft X-ray Transients in Quiescence
- X-ray irradiation in low mass binary systems
- Black Hole and Neutron Star Transients in Quiescence
- A radio-emitting outflow in the quiescent state of A0620-00: implications for modelling low-luminosity black hole binaries
- An Accretion-Jet Model for Black Hole Binaries: Interpreting the Spectral and Timing Features of XTE J1118+480
- White Dwarf Donors in Ultracompact Binaries: The Stellar Structure of Finite Entropy Objects
- The quiescent light curve and evolutionary state of GRO J1655-40
- Optical spectra of the carbon-oxygen accretion discs in the ultra-compact X-ray binaries 4U 0614+09, 4U 1543-624 and 2S 0918-549
- Advection-dominated accretion: global transonic solutions
- HST Fine Guidance Sensor Astrometric Parallaxes for Three Dwarf Novae: SS Aurigae, SS Cygni, and U Geminorum
- The origin and fate of short-period low-mass black-hole binaries
- Disc instability models for X-ray transients: evidence for evaporation and low alpha-viscosity ?
- Delays in dwarf novae I: The case of SS Cygni
- The Masses and Evolutionary State of the Stars in the Dwarf Nova SS Cygni
- Coronal X-Ray Emission from the Stellar Companions to Transiently Accreting Black Holes
- The cold neutron star in the soft X-ray transient 1H 1905+000
- XMM-Newton observations of two black hole X-ray transients in quiescence
- VY Sculptoris stars as magnetic CVs
- A Population of Faint Non-Transient Low Mass Black Hole Binaries
- The neutron star soft X-ray transient 1H1905+000 in quiescence
- On the distance of GRO J1655-40
- The dwarf nova SS Cygni: what is wrong?
- Implications of the HST/FGS parallax of SS Cygni on the disc instability model
- XMM-Newton observations of two transient millisecond X-ray pulsars in quiescence
- The formation of the coronal flow/ADAF
- X-ray Novae and the Evidence for Black Hole Event Horizons
- Physics of accretion flows around compact objects
- An XMM-Newton observation of the neutron star X-ray transient 2S 1803-245 in quiescence
- On the "failure" of the standard model for Soft X-ray Transients in quiescence
- Models of Soft X-Ray Transients and Dwarf Novae
Cited by in corpus (20)
- Foundations of Black Hole Accretion Disk Theory
- Stability of helium accretion discs in ultracompact binaries
- The evolution of ultracompact X-ray binaries
- Testing the disk instability model of cataclysmic variables
- An accurate geometric distance to the compact binary SS Cygni vindicates accretion disc theory
- Investigating the disc-jet coupling in accreting compact objects using the black hole candidate Swift J1753.5-0127
- Disk reflection and a possible disk wind during a soft X-ray state in the neutron star low-mass X-ray binary 1RXS J180408.9-342058
- The Galactic Bulge Survey: completion of the X-ray survey observations
- SWIFT XRT Observations of the Nova-like Cataclysmic Variables MV Lyr, BZ Cam and V592 Cas
- An Anomalous Quiescent Stellar Mass Black Hole
- Evolutionary models of short-period soft X-ray transients: comparison with observations
- Accretion Flows in Nonmagnetic White Dwarf Binaries as Observed in X-rays
- A late jet rebrightening revealed from multi-wavelength monitoring of the black hole candidate XTE J1752-223
- An X-ray-UV correlation in Cen X-4 during quiescence
- Outbursts of the intermediate-mass black hole HLX-1: a wind instability scenario
- What is the closest black hole to the Sun?
- The X-ray quiescence of Swift J195509.6+261406 (GRB 070610): an optical bursting X-ray binary?
- Variability of Optical Counterparts in the Chandra Galactic Bulge Survey
- Decade time-scale modulation of low mass X-ray binaries
- Quiescent NIR and optical counterparts to candidate black hole X-ray binaries