Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
University of Virginia
Univ. Virginia
Ecole Normale Superieure
ENS, Paris
Dept. of Astronomy, University of Virgina
Dept. of Astronomy, University of Virginia
UVa
Virginia, University, Charlottesville
University of Toronto, Toronto, Ontario, Canada
Laboratoire de Radio Astronomie, Ecole Normale Superieure, 24 rue Lhomond, 75231 Paris EDEX 05, France de Radioastronomie, École Normale Supérieure, 24 rue Lhomond, 75231 Paris, Cedex 05, France
Virginia Univ., Charlottesville.
Virginia Univ., Charlottesville
Laboratoire de Radioastronomie, École Normale Supérieure, 24 rue Lhomond, 75231 Paris Cedex 05, France; Institut Universitaire de France, Maison des Universités, 103 blvd. Saint-Michel, 75005 Paris, France
Leander McCormick Observatory, Charlottesville, VA
Steven A. Balbus is at the Laboratoire de Radioastronomie, École Normale Supérieure, 24 rue Lhomond, 75231 Paris cedex 05, France
Department of Astronomy, University of Virginia, PO Box 3818, Charlottesville, VA 22903, USA
Virginia Institute for Theoretical Astronomy, Department of Astronomy, University of Virginia, Charlottesville, Virginia 22903-0818
Virginia Institute of Theoretical Astronomy, Department of Astronomy, University of Virginia, Charlottesville, Virginia 22903
Virginia Institute of Theoretical Astronomy, Department of Astronomy, University of Virginia, Charlottesville, Virginia 22903-0818
Princeton University, New Observatory, NJ
U.Virginia
Ecole Normale Superieure and U. Virginia
University of Virginia Astronomy
Virginia Institute of Theoretical Astronomy, Department of Astronomy, University of Virginia, Charlottesville, VA 22903, USA
École Normale Supérieure, France
Princeton University, New Observatory, Princeton, NJ
California, University, Berkeley, CA
MIT, Cambridge, Mass.
Princeton University Observatory, NJ
MIT, Cam
A comparison of local simulations and reduced models of MRI-induced turbulence
A flux-limited treatment for the conductive evaporation of spherical interstellar gas clouds
A limitation of the generation of magnetic fields
A Magnetohydrodynamic Nonradiative Accretion Flow in Three Dimensions
A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution
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