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20052025
most citedThe Two Modes of Gas Giant Planet Formation

277 citations · 2.7k across the 67 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.EP2013★ 118 cited

Giant Planet Formation, Evolution, and Internal Structure

Ravit Helled, Peter Bodenheimer, Morris Podolak +7

The large number of detected giant exoplanets offers the opportunity to improve our understanding of the formation mechanism, evolution, and interior structure of gas giant planets…

astro-ph.EP2013★ 54 cited

High-Temperature Processing of Solids Through Solar Nebular Bow Shocks: 3D Radiation Hydrodynamics Simulations with Particles

A. C. Boley, M. A. Morris, S. J. Desch

A fundamental, unsolved problem in Solar System formation is explaining the melting and crystallization of chondrules found in chondritic meteorites. Theoretical models of chondrul…

astro-ph.EP2013★ 18 cited

The Formation of Systems with Tightly-packed Inner Planets (STIPs) via Aerodynamic Drift

Aaron C. Boley, Eric B. Ford

The NASA Kepler mission has revealed an abundant class of Systems with Tightly-packed Inner Planets (STIPs). The current paradigm for planet formation suggests that small planetesi…

astro-ph.SR2013★ 53 cited

Simulated Observations of Young Gravitationally Unstable Protoplanetary Discs

T. A. Douglas, P. Caselli, J. D. Ilee +4

The formation and earliest stages of protoplanetary discs remain poorly constrained by observations. ALMA will soon revolutionise this field. Therefore, it is important to provide…

astro-ph.EP2013★ 56 cited

The Evolution of Circumplanetary Disks around Planets in Wide Orbits: Implications for Formation Theory, Observations, and Moon Systems

Megan Shabram, Aaron Boley

Using radiation hydrodynamics simulations, we explore the evolution of circumplanetary disks around wide-orbit proto-gas giants. At large distances from the star (~100 AU), gravita…

astro-ph.EP2013★ 49 cited

Influence of viscosity and the adiabatic index on planetary migration

B. Bitsch, A. Boley, W. Kley

The strength and direction of migration of low mass embedded planets depends on the disk's thermodynamic state, where the internal dissipation is balanced by radiative transport, a…