Cover Image

Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	Gurrutxaga, Nerea, Johansen, Anders, Lambrechts, Michiel, Appelgren, Johan
Format:	Preprint
Published:	2023
Subjects:	Earth and Planetary Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

The evolution of the flux-size relationship in protoplanetary discs by viscous evolution and radial pebble drift
by: Appelgren, Johan, et al.
Published: (2025)

Thermal processing of primordial pebbles in evolving protoplanetary disks
by: Colmenares, Maria Jose, et al.
Published: (2024)

How the presence of a giant planet affects the outcome of terrestrial planet formation simulations
by: Kong, Zhihui, et al.
Published: (2024)

From planetesimals to planets with N-body simulations in the giant-planet formation region
by: Lorek, Sebastian, et al.
Published: (2026)

Interior dynamics of envelopes around disk-embedded planets
by: Kuwahara, Ayumu, et al.
Published: (2026)

UV-processing of icy pebbles in the outer parts of VSI-turbulent disks
by: Flores-Rivera, Lizxandra, et al.
Published: (2024)

mcdust: A 2D Monte Carlo code for dust coagulation in protoplanetary disks
by: Vaikundaraman, Vignesh, et al.
Published: (2025)

A Monte Carlo method for tracking dust properties during coagulation in protoplanetary disks
by: Gurrutxaga, Nerea, et al.
Published: (2026)

A break in planet occurrence near the pebble isolation mass should be observable by the Roman microlensing survey
by: Danti, Claudia, et al.
Published: (2026)

Comment on "Did the terrestrial planets of the Solar System form by pebble accretion?"
by: Johansen, Anders, et al.
Published: (2024)

Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds
by: Lorek, Sebastian, et al.
Published: (2024)

Evolution of gas envelopes and outgassed atmospheres of rocky planets formed via pebble accretion
by: Tomberg, Piia Maria, et al.
Published: (2024)

Dust ring and gap formation by gas flow induced by low-mass planets embedded in protoplanetary disks $\rm II$. Time-dependent model
by: Kuwahara, Ayumu, et al.
Published: (2024)

Vapor equilibrium models of accreting rocky planets demonstrate direct core growth by pebble accretion
by: Steinmeyer, Marie-Luise, et al.
Published: (2024)

Can the giant planets of the Solar System form via pebble accretion in a smooth protoplanetary disc?
by: Lau, Tommy Chi Ho, et al.
Published: (2024)

Gas dynamics around a Jupiter-mass planet I. Influence of protoplanetary disk properties
by: Lega, E., et al.
Published: (2024)

Clusters of tribocharged dust aggregates as pebbles in protoplanetary disks
by: Onyeagusi, F. C., et al.
Published: (2025)

How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
by: Houge, Adrien, et al.
Published: (2026)

The influence of dust growth on the observational properties of circumplanetary discs
by: Schulik, Matthäus, et al.
Published: (2025)

Formation of cold giant planets around late M dwarfs via core accretion and the fate of inner rocky worlds
by: Sanchez, Mariana, et al.
Published: (2025)

Gas dynamics around dust asymmetries in turbulent disks
by: Flores-Rivera, Lizxandra, et al.
Published: (2026)

The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks: Scale-dependence of dust diffusion
by: Schäfer, Urs, et al.
Published: (2025)

Three-dimensional transport of solids in a protoplanetary disk containing a growing giant planet
by: Van Clepper, Eric, et al.
Published: (2025)

A high-resolution survey of protoplanetary disks in Lupus and the nature of compact disks
by: Guerra-Alvarado, Osmar M., et al.
Published: (2025)

Fast formation of large ice pebbles after FU Orionis outbursts
by: Ros, Katrin, et al.
Published: (2024)

Burned to ashes: How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio
by: Houge, Adrien, et al.
Published: (2025)

Exploring the conditions for forming planetesimals by the streaming instability and planetary systems by pebble accretion
by: Johansen, Anders, et al.
Published: (2026)

Super-Earth formation in systems with cold giants
by: Danti, Claudia, et al.
Published: (2025)

The effect of dynamic temperatures on pebble dynamics and planet formation
by: Castrejon, Areli, et al.
Published: (2024)

Dust growth and pebble formation in the initial stages of protoplanetary disk evolution
by: Vorobyov, Eduard, et al.
Published: (2024)

Reproducing the stellar-mass dependence of the giant planet occurrence rate with pebble accretion models
by: Johnston, Heather F, et al.
Published: (2026)

Ices on pebbles in protoplanetary discs
by: Topchieva, A., et al.
Published: (2024)

Simulating the interplay between the snowline pebble flux and ongoing planet formation and migration
by: Astrakhantsev, Danila, et al.
Published: (2026)

Rocky planet formation in compact disks around M dwarfs
by: Sanchez, M., et al.
Published: (2024)

Formation of the Trappist-1 system in a dry protoplanetary disk
by: Schneeberger, Antoine, et al.
Published: (2024)

Fate of a remnant solid disk around an eccentric giant planet
by: Shibata, S., et al.
Published: (2024)

chemcomp: Modeling the chemical composition of planets formed in protoplanetary disks
by: Schneider, Aaron David, et al.
Published: (2023)

Modeling protoplanetary disk heating by planet-induced spiral shocks
by: Ono, Tomohiro, et al.
Published: (2024)

Carbonaceous Chondrites provide evidence for late-stage planetesimal formation in a pressure bump
by: Gurrutxaga, Nerea, et al.
Published: (2026)

Journey of complex organic molecules: Formation and transport in protoplanetary disks
by: Couzinou, T. Benest, et al.
Published: (2024)