Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Department of Astronomy, Indiana University, 727 East 3rd Street, Swain West 319, Bloomington, IN 47405, USA
Indiana University, Bloomington
Indiana Univ., Bloomington.
Astronomy Department, Indiana University, Bloomington, IN 47405, USA
Department of Astronomy, Indiana University, Bloomington, IN 47405
Department of Astronomy, Indiana University, 727 East Third Street, Bloomington, IN 47405, USA
Indiana University, Bloomington, Indiana, US
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany; Department of Astronomy, SW319, Indiana University, Bloomington, Indiana 47405, USA
Indiana Univ., Bloomington; Max-Planck-Inst. für extraterrestrische Physik, Garching bei München, Germany
Department of Astronomy, Indiana University, Bloomington, Indiana
Indiana University, Bloomington, IN
Department of Astronomy, Indiana University, Bloomington, IN 47405 Univ., CA.
Department of Astronomy, Indiana University, Swain Hall West 319, 727 East 3rd Street, Bloomington, IN 47405 of Astronomy, Indiana University, 727 E. 3rd St., Bloomington, IN 47405-7104, USA
Department of Astronomy, Indiana University, Bloomington, IN
Department of Astronomy, Indiana University, Bloomington, Indiana 47405, USA
Department of Astronomy, Swain West 319, 727 East 3rd Street, Indiana University, Bloomington, IN 47405-7105 ; Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany of Astronomy, Swain Hall West 319, Indiana University, Bloomington, IN 47405
NASA Ames Research Center
Indiana University, Bloomington, Ind.
NASA, Ames Research Center, Theoreti
3D Radiative Hydrodynamics for Disk Stability Simulations: A Proposed Testing Standard and New Results
3D Radiative Hydrodynamics Simulations of Protoplanetary Disks: A Comparison Between Two Radiative Cooling Algorithms
A Comparison of Saturn's Eletrostatic Discharges with Lightening on Various Planets.
A Dynamic m=1 Instability in Rapidly Rotating Low Mass Protostar Models
A hybrid scenario for gas giant planet formation in rings
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