Planet migration in three-dimensional radiative discs

DOI10.1051/0004-6361/200912072zbMath1181.85015arXiv0908.1863OpenAlexW2164944591WikidataQ68677411 ScholiaQ68677411MaRDI QIDQ3401277

W. Kley, B. Bitsch, H. Klahr

Publication date: 29 January 2010

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0908.1863

zbMATH Keywords

radiative transferhydrodynamicsaccretionaccretion disksplanets and satellites: formation

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (2)

TRHD: Three-temperature radiation-hydrodynamics code with an implicit non-equilibrium radiation transport using a cell-centered monotonic finite volume scheme on unstructured-grids ⋮ Theory and applications of fast Lyapunov indicators to model problems of celestial mechanics

Uses Software

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