30 citations · 54 across the 6 of their papers we have counts for
6 papers
Origin of the asymmetric gas distribution near the co-orbital Lagrange points of an embedded planet
Agustin Heron, Cristobal Petrovich, Pablo Benítez-Llambay +1
Hydrodynamic simulations of planet-disk interactions often show material accumulation near the co-orbital Lagrange points and -- features that may correspond to observe…
Ionized envelopes around protoplanets and the role of radiative feedback in gas accretion
Matías Montesinos, Juan Garrido-Deutelmoser, Jorge Cuadra +5
Planetary growth within protoplanetary disks involves accreting material from their surroundings, yet the underlying mechanisms and physical conditions of the accreting gas remain…
A Fast second-order solver for stiff multifluid dust and gas hydrodynamics
Leonardo Krapp, Juan Garrido-Deutelmoser, Pablo Benítez-Llambay +1
We present MDIRK: a Multifluid second-order Diagonally-Implicit Runge-Kutta method to study momentum transfer between gas and an arbitrary number () of dust species. The method…
A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain
Juan Garrido-Deutelmoser, Cristobal Petrovich, Carolina Charalambous +2
ALMA observations of the disk around HD 163296 have resolved a crescent-shape substructure at around 55 au, inside and off-center from a gap in the dust that extends from 38 au to…
Substructures in protoplanetary disks imprinted by compact planetary systems
Juan Garrido-Deutelmoser, Cristobal Petrovich, Leonardo Krapp +2
The substructures observed in protoplanetary disks may be the signposts of embedded planets carving gaps or creating vortices. The inferred masses of these planets often fall in th…
Dust trapping around Lagrangian points in protoplanetary disks
Matias Montesinos, Juan Garrido-Deutelmoser, Johan Olofsson +5
Trojans are defined as objects that share the orbit of a planet at the stable Lagrangian points and . In the Solar System, these bodies show a broad size distribution ra…