Hard X-rays from accretion disk boundary layers
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- Type
- article
- Published
- 1993-04-29
- Cited by
- 113
- References
- 15
- OpenAlex
- https://openalex.org/W2019779602
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:4365297
Keywords
Accretion (finance), Physics, Astrophysics, Intermediate polar, Boundary layer
References
- X-ray emission from cataclysmic variables with accretion disks. II. EUV/Soft x-ray radiation
- A flux-limited model of particle diffusion and viscosity
- Optical excess emission in T Tauri stars
- Vertical structure of accretion disks: A simplified analytical model
- Does accretion cease when a star approaches breakup
- A polytropic model of an accretion disk, a boundary layer, and a star
- Accretion Disks around T Tauri Stars
- Supersonic infall and causality in accretion disk boundary layers
- Hard X-ray spectrum of Cyg X-1
- Slim Accretion Disks
- X-ray emission from cataclysmic variables with accretion disks. I - Hard X-rays. II - EUV/soft X-ray radiation
- Accretion Discs in Astrophysics
- Black Holes in the Galaxy
- BLACK HOLE MODELS FOR ACTIVE GALACTIC NUCLEI
- A two-temperature accretion disk model for Cygnus X-1: structure and spectrum.
Cited by
- The Radial-Azimuthal Instability of Gas-Pressure-Dominated Accretion Disk with Advection
- Modelling the black hole silhouette in Sagittarius A* with ion tori
- Disc Instabilities and “Soft” X-Ray Transients
- Boundary Layers in Cataclysmic Variables and Pre-Main-Sequence Stars
- SWIFT X-RAY TELESCOPE OBSERVATIONS OF THE NOVA-LIKE CATACLYSMIC VARIABLES MV Lyr, BZ Cam, AND V592 Cas
- Chandra Detection of the AM Canum Venaticorum Binary ES Ceti (KUV 01584–0939)
- On the boundary layer of accretion discs
- Transition from radiatively inefficient to cooling dominated phase in two temperature accretion disks around black holes
- ON HYDROMAGNETIC STRESSES IN ACCRETION DISK BOUNDARY LAYERS
- X–ray observations of accreting white–dwarf systems
- Resolving different sources of fast X-ray variability of the dwarf nova RU Peg in quiescence
- The X-Ray Spectral Analysis of Dwarf Nova WZ Sge Observed with ROSAT in Quiescence
- Heating of a Star by Disk Accretion
- Thermal equilibria of accretion discs around black holes: a review of the recent progress
- The Nature of the Hard X-Ray-Emitting Symbiotic Star RT Cru
- Rms–flux relation and fast optical variability simulations of the nova-like system MV Lyr
- Numerical Models of Viscous Accretion Flows near Black Holes
- Advection in Accretion Disk Boundary Layers
- Preliminary results of the spectral analysis of Suzaku data of SW Ursae Majoris and BZ Ursae Majoris
- The X-Ray Eclipse of the Dwarf Nova HT Cassiopeiae: Results from ASCA and ROSAT HRI Observations
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