12 citations · 27 across the 18 of their papers we have counts for
7 papers · 1 filter
Star Planet Interactions
Arghyadeep Paul, Kristina Kislyakova, Manuel Güdel +13
Star-planet interactions (SPIs) describe the continuous exchange of energy, momentum, and mass between exoplanets and their host stars through radiative, tidal, magnetic, and parti…
Launching of asymmetric outflows from the star-disk magnetosphere
Miljenko Čemeljić, Aleksandra Kotek, Włodek Kluźniak
In resistive and viscous magnetohydrodynamical simulations, we obtain axial outflows launched from the innermost magnetosphere of a star-disk system. The launched outflows are foun…
Backflow in simulated MHD accretion disks
Ruchi Mishra, Miljenko Čemeljić, Wlodek Kluźniak
We perform resistive MHD simulations of accretion disk with alpha-viscosity, accreting onto a rotating star endowed with a magnetic dipole. We find backflow in the presence of stro…
Backflow in Accretion Disk
Ruchi Mishra, Miljenko Čemeljić, Wlodek Kluźniak
Analytical solution for a thin hydrodynamic accretion disk shows that for some values of the viscosity parameter part of the accretion flow in the disk is not towards the star, but…
Transport of dust grain particles in the accretion disk
Robert Jaros, Miljenko Čemeljić, Włodek Kluźniak +2
Entrainment of dust particles in the flow inside and outside of the proto-planetary disk has implications for the disk evolution and composition of planets. Using quasi-stationary…
Light curve variation caused by accretion column switching stellar hemispheres
Miljenko Čemeljić
I use two-dimensional axisymmetric numerical simulations of star-disk magnetospheric interaction to construct a three-dimensional model of hot spots on the star created by infallin…
"Atlas" of numerical solutions for star-disk magnetospheric interaction
Miljenko Čemeljić
Aims: I report results in numerical simulations of star-disk magnetospheric interaction. A thin accretion disk with corona above a rotating stellar surface is simulated in a parame…