Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Univ. Bern, Switzerland
Institute of Physics, University of Berne, Sidlerstr. 5, Bern, 3012 Switzerland Center for Astrophysics, Cambridge, MA
Los Alamos National Laboratory, NM; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Physikalisches Institut, University of Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
Bern, Swtizerland
Bern University, Switzerland
U. Bern
Arizona Univ., Tucson, AZ
Physikalisches Institut, Universität Bern, Sidlerstrasse 5, CH-3012 Bern, Switzerland
Geneve, Observatoire, Sauverny, Switzerland
University of Bern
University of Bern, Physikalisches Institut, Sidlerstrasse 5, 3012 Bern, Switzerland
University of Berne, Institute of Physics, Space Research and Planetary Science, Sidlerstr. 5, CH - 3012 Berne, Switzerland, Institut Universität Bern, Sidlerstrasse 5, 3012 Bern, Switzerland
Department des Etudes Spatiales, Institut de Physique du Globe de Paris, 4 Avenue de Neptune, 94100 Saint Maur des Fossés Cedex, France, FRInstitute of Geophysics, ETH-Hönggerberg, CH-9093 Zürich, Switzerland, CHJet Propulsion Laboratory, California Institut of Technology, 4800 Oak Grove Dr. Pasadena, CA 91109, USA, USLaboratoire de Planétologie et Géodynamique, Faculté des Sciences et des Techniques, 2, Rue de la Houssinière, BP92 208, 44322 Nantes Cedex, France, FRInstitute of Planetology, Wilhelm-Klemm Str. 10, D-48149 Münster, Germany, DEDepartment de Sismologie, Institut de Physique du Globe de Paris, 4 Place Jussieu, 75252 Paris Cedex 05, France, FRCentre de Recherche Géophysique, Institut National des Sciences de l'Univers, Garchy, France, FRLaboratoire de Géophysique Interne et de Tectonophysique Observatoire de Grenoble, IRIGM, BP53X 38041 Grenoble Cedex, France, FRUMR Géosciences Azur, 250 rue A. Einstein, 06560 Valbonne, F
3D models of rotating magnetic gas clouds. I - Time evolution, mass spectrum and angular momentum
4 stars with long-period planets (Dumusque+, 2011)
A comparison between SPH and PPM: simulations of stellar collisions
A comprehensive set of simulations of high-velocity collisions between main sequence stars
A Consistent Model of Planet Formation and Differentiation: Implications from Monte-Carlo Simulations and Computational Fluid Dynamics
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