Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Texas
University of Texas at Austin
University of Texas at Austin;
University of Texas, Austin
Department of Astronomy, University of Texas at Austin
UT Austin
Univ. of Texas at Austin
U. of Texas
The University of Texas at Austin
UTexas, Austin
Department of Astronomy, University of Texas, Austin, USA
University of Texas-Austin
Dept. of Astronomy, University of Texas, Austin
Univ. Texas at Austin
Dept. Astronomy, U. Texas Austin
Dept. of Astronomy, The University of Texas at Austin
UTAustin
Texas, TCC
ChosunU
U Texas at Austin
Texas, University, Austin
University of Texas, Austin, TX, US
Department of Astronomy, 1 University Station, C1400, Austin TX 78712
Texas Cosmology Center, University of Texas, Austin, TX 78712, USA; Department of Astronomy, University of Texas, Austin, TX 78712, USA
Department of Astronomy and Texas Cosmology Center, The University of Texas at Austin, USA
Department of Astronomy, University of Texas, Austin, Texas 78712Jens V.VillumsenKarl-Schwarzschild-Str. 1, Postfach 15 23, 85740 Garching bei München, Germany
Texas Univ., Austin.
Texas Univ., Austin
UTexas
Harvard College Observatory and Smithsonian Astrophysical Observatory, Cambridge, Mass.
Department of Astronomy, University of Texas, Austin, Texas, USA of Astronomy, University of Texas, Austin, Texas, USA
Stanford University, Stanford, Calif.
Institute for Advanced Study, Princeton, N.J.
UT-Austin
Harvard-Smithsonian Center for Astrophysics, Cambridge, Mass.
Texas, University, Austin, TX
Harvard University, Cambridge, Mass.
Smithsonian Astrophysical Observatory and Harvard College Observatory, Cambridge, Mass.
A Convenient Set of Comoving Cosmological Variables and Their Application
A Model for the Formation and Evolution of Cosmological Haloes
A Model for the Formation and Evolution of Cosmological Halos
A Model for the Optical Behavior of Grains with Resonant Impurities
A model for the postcollapse equilibrium of cosmological structure: truncated isothermal spheres from top-hat density perturbations
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