Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
U. Texas
University of Texas
Johns Hopkins Univ.
The University of Texas at Austin
McMaster U
JHU
Texas, University, Austin
Texas Univ., Austin.
Texas University
Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles St., Baltimore, MD 21218, USA of Texas, Austin
Korea Astronomy Observatory, Daejon, Korea
McMaster University, Canada
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, US
Johns Hopkins University
Department of Physics and Astronomy, McMaster University, 1280 Main St. West, Hamilton, ON L8S 4M1, Canada
Astronomy Department, University of Texas, Austin, Texas 78712
Texas, University; McDonald Observatory, Austin
Department of Physics and Astronomy, The Johns Hopkins University, Baltimore, MD 21218, USA
Editor-in-Chief
Department of Astronomy, University of Texas, Austin
Department of Astronomy, University of Texas at Austin, Austin, Texas 78712
Department of Physics and Astronomy, Johns Hopkins University, 3400 N. Charles St., Baltimore, MD USA 21218
Texas Univ., Austin
Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MA, USA
University of Texas, Austin, TX, US
Department of Astronomy, University of Texas, Austin, Texas 78712
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
University of Texas, Austin, Austi, TX, US
UT Austin
John Hopkins
University of Texas, MIT, Harvard-Smithsonian CfA
Princeton University, Princeton, NJ
UT-Austin
Texas, University, Austin, TX
Johns Hopkins University, 3400 N. Charles St., Baltimore MD 21218
Princeton University, New Observatory, Princeton, NJ
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Princeton University, Princeton, NJ
Johns Hopkins University.
A Kinematic Dynamo Driven By Internal Waves In Accretion Disks
A Kinematic Dynamo in Accretion Disks
A linear stability analysis for wind-driven bubbles
A Local Instability In Accretion Disks and the Nature of α
A model for the distribution of the intergalactic medium
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