The accretion mechanism in low power radio-galaxies Ranieri D. Baldi 1, Barbara Balmaverde 2 & Alessandro Capetti 2 1: Università degli Studi di Torino.
What are ultraluminous X-ray sources? Tim Roberts.
Some issues on models of black hole X-ray binaries Feng Yuan Shanghai Astronomical Observatory, Chinese Academy of Sciences.
ADVECTION- DOMINATED ACCRETION Ramesh Narayan. Why Do We Need Another Accretion Model? Black Hole (BH) accretion is not as simple as people originally.
A.Kravtsov (U.Chicago) D. Ceverino (NMSU) O. Valenzuela (U.Washington) G. Rhee (UNLV) F. Governato, T.Quinn, G.Stinson (U.Washington) J.Wadsley (McMaster,
Luminous Hot Accretion Flows ------extending ADAF beyond its critical accretion rate Feng Yuan Shanghai Astronomical Observatory, Chinese Academy of Science.
Kravtsov (U.Chicago) D. Ceverino (NMSU)
Radiatively Inefficient Accretion Flows Roman Shcherbakov, 28 November, 2007.
1Propeller and Variability IGR J18245-2452 - C. FerrignoEWASS 26.06.2015 Numerical simulations of propeller accretion regime and the variability of IGR.
Radiatively Inefficient Accretion Flows
Lecture 2 The role of BHs in AGN Basic concepts of the standard model of AGN Evidence for BHs in AGN Methods to weight a BH in an AGN Demographics of QSOs.
The accretion mechanism in low power radio-galaxies
