Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Univ. of Chicago
Dept. of Astronomy and Astrophysics, Univ. of Chicago
Depts. of Astronomy & Astrophysics and of Physics, The University of Chicago
U. of Chicago
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Enrico Fermi Institute, The University of Chicago 5640 South Ellis Avenue, Chicago, IL 60637; Argonne National Laboratory, 9700 South Cass Avenue, Argonne, IL 60439 Center for Astrophysics, Cambridge, Mass.
At the Harvard-Smithsonian Center for Astrophysics.
Chicago, University, IL
Astronomy and Astrophysics and Enrico Fermi Institute, The University of Chicago at Chicago
Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, Mass.
Department of Physics, The University of Chicago, Chicago, Illinois 60637; Center for Astrophysical Thermonuclear Flashes, The University of Chicago, Chicago, Illinois 60637; Department of Astronomy & Astrophysics, The University of Chicago, Chicago, Illinois 60637; and Enrico Fermi Institute, The University of Chicago, Chicago, Illinois 60637
Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637, USA
U.Chicago; CfA
University of Chicago, Chicago, IL
ASCI Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, Illinois
Department of Astronomy and Astrophysics, and Enrico Fermi Institute, University of Chicago, Chicago, IL 60637
ASCI Flash Center / University of Chicago
Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL 60637; Center for Astrophysical Thermonuclear Flashes, University of Chicago, Chicago, IL 60637; Enrico Fermi Institute, University of Chicago, Chicago, IL 60637.
Departments of Astronomy and Astrophysics and Physics, The University of Chicago, Chicago, Illinois 60637
Department of Astronomy and Astrophysics, University of Chic
'Coronae' of rotating interstellar clouds
A computational code for two-dimensional unsteady magnetohydrodynamics by the method of characteristics
A glimpse of new results - The preliminary Solar Maximum Mission data
A heating mechanism for the chromospheres of M dwarf stars
A magnetohydrodynamic model for Herbig-Haro objects - Magnetically guided shocked flows associated with optical jets from young stellar objects
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Profile ID: LFWR-SCP-P-26575