Add to ORKGIn the core accretion model, gas giant formation is a race between growth and migration; for a core to become a jovian planet, it must accrete its envelope before it spirals into the host star. We use a multizone numerical model to extend our previous investigation of the "window of opportunity" for gas giant formation within a disk. When the collision cross-section enhancement due to core atmospheres is taken into account, we find that a broad range of protoplanetary disks posses such a window
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. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
In the core-accretion model, gas-giant planets form solid cores which then accrete gaseous envelopes...
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...
We present evolutionary models of gas giant planets forming in protoplanetary disks. We first consid...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
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...
This thesis describes efforts to improve the realism of numerical models of giant planet formation a...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
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. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
In the core-accretion model, gas-giant planets form solid cores which then accrete gaseous envelopes...
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...
We present evolutionary models of gas giant planets forming in protoplanetary disks. We first consid...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
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...
This thesis describes efforts to improve the realism of numerical models of giant planet formation a...
Context. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...
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. In the classical core-accretion planet-formation scenario, rapid inward migration and accre...