Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Scientist
OCA
Laboratoire Cassiopée, Centre National de la Recherche Scientifique, UMR 6202, Observatoire de la Côte d'Azur, BP 4229, 06304 Nice Cedex 4, France of Physics, University of Tubingen, Germany
Université de Nice Sophia-antipolis / Observatoire de la Côte d'Azur, boulevard de l'Observatoire, BP4229, 06304, NICE cedex 4, France
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, UK
Cambridge University - DAMTP, United Kingdom
Observatoire de la Côte d'Azur, France
Institut für Astronomie und Astrophysik, Universität Túbingen, Auf der Morgenstelle 10, 72076 Tübingen, Germany
Université de Nice Sophia-antipolis / CNRS / Observatoire de la Côte d'Azur, Boulevard de l'Observatoire, BP 4229, 06304 NICE Cedex 4, FRANCE ; Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Centre for Mathematical Sciences, Wilberforce Road, Cambridge CB3 0WA, UK
Université de Nice Sophia-antipolis, Observatoire de la Côte d'Azur, Cassiopée, NICE cedex 4, France
Universiy of Tuebingen
CASSIOPEE
Observatoire de la Côte d'Azur, B.P. 4229, 06304 Nice Cedex 4, France
Observatoire de la Cote d'Azur, France
Aurélien Crida is at the Laboratoire Cassiopée, Université de Nice Sophia-antipolis / CNRS / Observatoire de la Côte d'Azur - BP4229, 06304 Nice Cedex 4, France aurelien.
University of Cambridge, United Kingdom
Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, UK
University of Tübingen, Germany
A torque formula for non-isothermal Type I planetary migration - I. Unsaturated horseshoe drag
Accretion of Saturn's mid-sized moons during the viscous spreading of young massive rings: solving the paradox of silicate-poor rings versus silicate-rich moons
Are Saturn's inner satellites the children of Saturn's main rings ?
Building Giant-Planet Cores at a Planet Trap
Cavity formation in protoplanetary disks
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