3 papers
astro-ph.EP2025
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…
astro-ph.EP2025
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…
astro-ph.EP2020
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…