Add to ORKGIn the standard model of core accretion, the cores of the giant planets form by the accretion of planetesimals. In this scenario, the evolution of the planetesimal population plays an important role in the formation of massive cores. Recently, we studied the role of planetesimal fragmentation in the in situ formation of a giant planet. However, the exchange of angular momentum between the planet and the gaseous disk causes the migration of the planet in the disk. In this new work, we incorporate the migration of the planet and study the role of planet migration in the formation of a massive core when the population of planetesimals evolves by planet accretion, migration, and fragmentatio
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
Context. Most planet formation models that incorporate planetesimal fragmentation consider a catastr...
In the standard model of core accretion, the cores of the giant planets form by the accretion of pla...
In the standard model of core accretion, the cores of the giant planets form by the accretion of pla...
In the standard model of core accretion, the cores of the giant planets form by the accretion of pla...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
In the core-accretion model, gas-giant planets form solid cores which then accrete gaseous envelopes...
We develop a simple model for computing planetary formation based on the core instability model for ...
Context. Most planet formation models that incorporate planetesimal fragmentation consider a catastr...
We extend the core-accretion model of giant gaseous planets by Pollack et al. ([CITE]) to include mi...
We extend the core-accretion model of giant gaseous planets by Pollack et al. ([CITE]) to include mi...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
Context. Most planet formation models that incorporate planetesimal fragmentation consider a catastr...
In the standard model of core accretion, the cores of the giant planets form by the accretion of pla...
In the standard model of core accretion, the cores of the giant planets form by the accretion of pla...
In the standard model of core accretion, the cores of the giant planets form by the accretion of pla...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
Context. In the standard scenario of planet formation, terrestrial planets and the cores of the gian...
In the core-accretion model, gas-giant planets form solid cores which then accrete gaseous envelopes...
We develop a simple model for computing planetary formation based on the core instability model for ...
Context. Most planet formation models that incorporate planetesimal fragmentation consider a catastr...
We extend the core-accretion model of giant gaseous planets by Pollack et al. ([CITE]) to include mi...
We extend the core-accretion model of giant gaseous planets by Pollack et al. ([CITE]) to include mi...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
Context. Most planet formation models that incorporate planetesimal fragmentation consider a catastr...