activity
20032023
most citedMagnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations

16 citations · 32 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2023★ 3 cited

Trends in torques acting on the star during a star-disk magnetospheric interaction

M. Čemeljić, A. S. Brun

We assess the modification of angular momentum transport in various configurations of star-disk accreting systems based on numerical simulations with different parameters. We quant…

astro-ph.SR2023★ 5 cited

Magnetically threaded accretion disks in resistive magnetohydrodynamic simulations and asymptotic expansion

Miljenko Čemeljić, Włodek Kluźniak, Varadarajan Parthasarathy

Aims. A realistic model of magnetic linkage between a central object and its accretion disk is a prerequisite for understanding the spin history of stars and stellar remnants. To t…

astro-ph.HE2020★ 1 cited

Flux ropes in SANE disks

Miljenko Čemeljić, Feng Yuan, Hai Yang

Three-dimensional numerical simulations of a hot accretion flow around a supermassive black hole are performed using the general relativity magneto-hydrodynamic (GRMHD) code Athena…

astro-ph.HE2018★ 3 cited

MHD simulations of resistive viscous accretion disk around millisecond pulsar

M. Čemeljić, V. Parthasarathy, W. Kluźniak

We perform MHD simulations of a thin resistive and viscous accretion disk around a neutron star with the surface dipolar magnetic field of 10 Gauss. The system evolution is fol…

astro-ph.SR2014★ 4 cited

Large resistivity in numerical simulations of radially self-similar outflows

Miljenko Čemeljić, Nektarios Vlahakis, Kanaris Tsinganos

We investigate the differences between an outflow in a highly-resistive accretion disk corona, and the results with smaller or vanishing resistivity. For the first time, we determi…

astro-ph.SR2011★ 16 cited

Magnetospheric Accretion and Ejection of Matter in Resistive Magnetohydrodynamic Simulations

Miljenko Čemeljić, Hsien Shang, Tzu-Yang Chiang

The ejection of matter in the close vicinity of a young stellar object is investigated, treating the accretion disk as a gravitationally bound reservoir of matter. By solving the r…