175 citations · 2.5k across the 90 of their papers we have counts for
5 papers · 2 filters
3D Radiation Non-ideal Magnetohydrodynamical Simulations Of The Inner Rim In Protoplanetary Disks
M. Flock, S. Fromang, N. J. Turner +1
Many planets orbit within an AU of their stars, raising questions about their origins. Particularly puzzling are the planets found near the silicate sublimation front. We investiga…
Can dead zones create structures like a transition disk?
Paola Pinilla, Mario Flock, Maria de Juan Ovelar +1
[Abridged] Regions of low ionisation where the activity of the magneto-rotational instability is suppressed, the so-called dead zones, have been suggested to explain gaps and asymm…
Magnetic fields in protoplanetary disks: from MHD simulations to ALMA observations
Gesa H. -M. Bertrang, Mario Flock, Sebastian Wolf
Magnetic fields significantly influence the evolution of protoplanetary disks and the formation of planets, following the predictions of numerous magnetohydrodynamic (MHD) simulati…
Radiation hydrodynamical models of the inner rim in protoplanetary disks
M. Flock, S. Fromang, N. J. Turner +1
Many stars host planets orbiting within a few astronomical units (AU). The occurrence rate and distributions of masses and orbits vary greatly with the host stars mass. These close…
Gaps, rings, and non-axisymmetric structures in protoplanetary disks - Emission from large grains
J. P. Ruge, M. Flock, S. Wolf +5
Dust grains with sizes around (sub)mm are expected to couple only weakly to the gas motion in regions beyond 10 au of circumstellar disks. In this work, we investigate the influenc…