S
S. Fromang
Researcher at University of Paris
Publications - 19
Citations - 1115
S. Fromang is an academic researcher from University of Paris. The author has contributed to research in topics: Magnetorotational instability & Turbulence. The author has an hindex of 13, co-authored 19 publications receiving 1031 citations. Previous affiliations of S. Fromang include Centre national de la recherche scientifique & Institut d'Astrophysique de Paris.
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Journal ArticleDOI
A comparative study of disc-planet interaction
M. de Val-Borro,Richard G. Edgar,Pawel Artymowicz,P. Ciecielag,P. Cresswell,Gennaro D'Angelo,E. J. Delgado-Donate,G. Dirksen,S. Fromang,A. Gawryszczak,Hubert Klahr,Wilhelm Kley,Wladimir Lyra,Frédéric Masset,Garrelt Mellema,Richard P. Nelson,Sijme-Jan Paardekooper,Adam Peplinski,A. Pierens,Tomasz Plewa,Ken Rice,C. Schaefer,Roland Speith +22 more
TL;DR: In this article, numerical simulations of a disc-planet system using various grid-based and smoothed particle hydrodynamics (SPH) codes are performed for a simple setup where Jupiter and Neptune mass planets on a circular orbit open a gap in a protoplanetary disc during a few hundred orbital periods.
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3D Radiation Nonideal Magnetohydrodynamical Simulations of the Inner Rim in Protoplanetary Disks
TL;DR: In this article, conditions near the front in the protostellar disk around a young intermediate-mass star were investigated using the first global 3D radiation non-ideal MHD simulations in this context.
Journal ArticleDOI
3D Radiation Non-ideal Magnetohydrodynamical Simulations Of The Inner Rim In Protoplanetary Disks
TL;DR: In this paper, conditions near the front in the protostellar disk around a young intermediate-mass star were investigated using the first global 3D radiation non-ideal MHD simulations in this context.
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On the aerodynamic redistribution of chondrite components in protoplanetary disks
TL;DR: In this paper, the dynamics of the solids, subject to gas drag, were found to be essentially controlled by the gas-solid decoupling parameter, i.e., the ratio of the dimensionless stopping time to the turbulence parameter.
Journal ArticleDOI
Radiation Magnetohydrodynamics In Global Simulations Of Protoplanetary Disks
TL;DR: In this paper, a radiative transfer method based on the flux-limited diffusion approximation that includes frequency dependent irradiation by the central star was developed for global 3D radiation MHD simulations of a stratified protoplanetary disk.