Abstract: By studying three-dimensional, radiative, global simulations of sub-Eddington, geometrically thin (H/R ≈ 0.15) black hole accretion flows we show that thin discs which are dominated by ...

This project explores the equations of the thin disk accretion model, considered with both Newtonian gravity and General Relativity (Novikov & Thorne, 1973). This README provides an overview of the ...

Here we present an alternative possibility, involving strong, unbound, magnetic coronae generated by geometrically thin, optically thick accretion discs at low accretion rates. First we show that, if ...

This project explores the equations of the thin disk accretion model, considered with both Newtonian gravity and General Relativity (Novikov & Thorne, 1973). This README provides an overview of the ...

In the case of V4142 Sgr, researchers conducted a detailed analysis of the binary's light curve and spectral data, revealing the presence of a geometrically thick accretion disk around the hotter ...