activity
20042026
most citedGRMHD Simulations of Magnetized Advection Dominated Accretion on a Non-Spinning Black Hole: Role of Outflows

504 citations · 5.2k across the 62 of their papers we have counts for

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Showing 2013 · astro-ph.HEShow all

8 papers · 2 filters

astro-ph.HE2013★ 336 cited

Numerical simulations of super-critical black hole accretion flows in general relativity

A. Sadowski, R. Narayan, J. C. McKinney +1

A new general relativistic radiation magnetohydrodynamical code KORAL, is described, which employs the M1 scheme to close the radiation moment equations. The code has been successf…

astro-ph.HE2013★ 18 cited

Simulating the effect of the Sgr A* accretion flow on the appearance of G2 after pericenter

David Abarca, Aleksander Sadowski, Lorenzo Sironi

We study the dynamical interaction of the G2 cloud with the accretion flow around Sgr A* by means of three-dimensional, hydrodynamic simulations. We show the effects of the rotatin…

astro-ph.HE2013★ 11 cited

Inner Disc Obscuration in GRS 1915+105 Based on Relativistic Slim Disc Model

K. Vierdayanti, A. Sadowski, S. Mineshige +1

We study the observational signatures of the relativistic slim disc of 10 M_sun black hole, in a wide range of mass accretion rate, mdot, dimensionless spin parameter, a_ast, and v…

astro-ph.HE2013★ 110 cited

General Relativistic Magnetohydrodynamic Simulations of Blandford-Znajek Jets and the Membrane Paradigm

Robert F. Penna, Ramesh Narayan, Aleksander Sadowski

Recently it has been observed that the scaling of jet power with black hole spin in galactic X-ray binaries is consistent with the predictions of the Blandford-Znajek (BZ) jet mode…

astro-ph.HE2013★ 196 cited

Energy, momentum and mass outflows and feedback from thick accretion discs around rotating black holes

A. Sadowski, R. Narayan, R. Penna +1

Using long-duration general relativistic magnetohydrodynamic simulations of radiatively inefficient accretion discs, the energy, momentum and mass outflow rates from such systems a…

astro-ph.HE2013★ 27 cited

Location of the bow shock ahead of cloud G2 at the Galactic Center

A. Sadowski, R. Narayan, L. Sironi +1

We perform detailed magnetohydrodynamic simulations of the gas cloud G2 interacting with the accretion flow around the Galactic Center black hole Sgr A*. We take as our initial con…

astro-ph.HE2013★ 195 cited

Semi-implicit scheme for treating radiation under M1 closure in general relativistic conservative fluid dynamics codes

Aleksander Sadowski, Ramesh Narayan, Alexander Tchekhovskoy +1

A numerical scheme is described for including radiation in multi-dimensional general-relativistic conservative fluid dynamics codes. In this method, a covariant form of the M1 clos…

astro-ph.HE2013★ 49 cited

Radio light curves during the passage of cloud G2 near Sgr A*

A. Sadowski, L. Sironi, D. Abarca +3

We calculate radio light curves produced by the bow shock that is likely to form in front of the G2 cloud when it penetrates the accretion disk of Sgr A*. The shock acceleration of…