@inbook{a854e86faed340afb36c75f5d799d5cd,
title = "Conditions for outward migration",
abstract = "The migration of protoplanets in discs not only depends on the thermodynamics of the ambient disc but also on the orbital parameters of the embedded planet. In the fully radiative regime, planets can migrate outward if their orbital parameters fit in a very small range. We simulate planets in fully radiative discs (and isothermal discs-for reference) and determine the influence of the orbital parameters (a, e and i) and the planetary mass on the migration time scale and direction.",
keywords = "Accretion disks, Hydrodynamics, Planetary systems: formation, Radiative transfer",
author = "Bertram Bitsch and Willy Kley",
year = "2010",
month = oct,
doi = "10.1017/S1743921311020953",
language = "English",
isbn = "9780521196529",
series = "Proceedings of the International Astronomical Union",
number = "S276",
pages = "497--498",
editor = "Alessandro Sozzetti and Mario Lattanzi and Alan Boss",
booktitle = "The Astrophysics of Planetary Systems",
edition = "S276",
}