Accretion Flows in X-ray Binaries
arXiv:astro-ph/0203246 · doi:10.1098/rsta.2002.1047
Abstract
I review the X-ray observations of Galactic accreting black holes and neutron stars, and interpretions of these in terms of solutions of the accretion flow equations.
13 pages; Philosophical Transactions of the Royal Society (Series A: Mathematical, Physical, and Engineering Sciences), submitted
References in corpus (12)
- The disc instability model of dwarf-novae and low-mass X-ray binary transients
- XMM-EPIC observation of MCG-6-30-15: Direct evidence for the extraction of energy from aspinning black hole?
- X-ray Reflection By Photoionized Accretion Discs
- Modeling the Low State Spectrum of the X-Ray Nova XTE J1118+480
- A Possible Explanation for the "Parallel Tracks" Phenomenon in Low-Mass X-Ray Binaries
- Observational Evidence for Strong Disk Comptonization in GRO J1655-40
- Local Axisymmetric Simulations of Magneto-Rotational Instability in Radiation-Dominated Accretion Disks
- A comment on the colour-colour diagrams of Low Mass X-ray Binaries
- Mapping the inner accretion disk of the galactic black hole J1550-564 through its rise to outburst
- A Complete Relativistic Ionized Accretion Disc in Cygnus X-1
- Testing models of X-ray reflection from irradiated disks
- Slim Disk: Viscosity Prescriptions and Observational Implications
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