The simulations presented in this paper utilized Queen Mary's MidPlus computational facilities, supported by QMUL Research-IT and funded by EPSRC grant EP/K000128/1. This research was supported in part by the National Science Foundation under Grant No. NSF PHY-1125915
We present a new computation of the linear tidal interaction of a protoplanetary core with a thin ga...
The formation of planets depends on the underlying protoplanetary disc structure, which in turn infl...
Massive planetary cores embedded in protoplanetary discs are believed to accrete extended atmosphere...
The core accretion hypothesis posits that planets with significant gaseous envelopes accreted them f...
We study a solid protoplanetary core of 1-10 earth masses migrating through a disk. We suppose the c...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
We know now that discs of gas and dust, so-called protoplanetary discs, form planets as side-product...
In the core accretion model, gas giant formation is a race between growth and migration; for a core ...
Received — ; accepted — The formation of planetary cores must proceed rapidly in order for the giant...
Gas giant planets may form early-on during the evolution of protostellar discs, while these are rela...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
The formation of planetary cores must proceed rapidly in order for the giant planets to accrete thei...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Abstract. We present evolutionary models of gas giant planets forming in protoplanetary disks. We fi...
We present a new computation of the linear tidal interaction of a protoplanetary core with a thin ga...
The formation of planets depends on the underlying protoplanetary disc structure, which in turn infl...
Massive planetary cores embedded in protoplanetary discs are believed to accrete extended atmosphere...
The core accretion hypothesis posits that planets with significant gaseous envelopes accreted them f...
We study a solid protoplanetary core of 1-10 earth masses migrating through a disk. We suppose the c...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. According to the sequential accretion model (or core-nucleated accretion model), giant plan...
We know now that discs of gas and dust, so-called protoplanetary discs, form planets as side-product...
In the core accretion model, gas giant formation is a race between growth and migration; for a core ...
Received — ; accepted — The formation of planetary cores must proceed rapidly in order for the giant...
Gas giant planets may form early-on during the evolution of protostellar discs, while these are rela...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
The formation of planetary cores must proceed rapidly in order for the giant planets to accrete thei...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Abstract. We present evolutionary models of gas giant planets forming in protoplanetary disks. We fi...
We present a new computation of the linear tidal interaction of a protoplanetary core with a thin ga...
The formation of planets depends on the underlying protoplanetary disc structure, which in turn infl...
Massive planetary cores embedded in protoplanetary discs are believed to accrete extended atmosphere...