Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Rice University
Now at Space Sciences Laboratory, University of California, Berkeley, CA 94720
Department of Physics and Astronomy, Rice University, Houston, TX 77005, USA
Physics and Astronomy Department, Rice University, Houston, TX 77005, USA
Department of Physics and Astronomy, Rice University, 6100 Main St. MS-108, Houston
Department of Physics and Astronomy, Rice University, Houston, TX, USA
Department of Physics and Astronomy, Rice University, Houston, TX 77005
Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106; Department of Physics and Astronomy, 6100 Main Street, Rice University, Houston, TX 77005.
Department of Physics and Astronomy, Rice University, 6100 Main Street, Houston, Texas 77005, USA
Space Sciences Laboratory, University of California, Berkeley, Berkeley, CA 94720 of Physics and Astronomy, Rice University, Mail Stop 108, 6100 Main Street, Houston, TX 77005 Sciences Laboratory, University of California at Berkeley, Berkeley, CA 94720 Sciences Laboratory, Berkeley, CA 94720 Science Laboratory, University of California, Berkeley, CA 94720-7450; Now at Department of Physics and Astronomy, Rice University, Houston, TX 77005.
Department of Physics and Astronomy, Rice University, 6100 Main Street, MS-108, Houston, TX 77005
Now at Space Sciences Laboratory, University of California, Berkeley, Berkeley, CA 94720
JILA
Department of Physics and Astronomy-MS 108, Rice University 6100 Main Street, Houston, TX 77005, USA
Department of Physics and Astronomy-MS 108 Rice University, 6100 Main Street Houston, TX 77005
JILA, University of Colorado, Boulder, CO, USA
Rice
McDonald Obs., Uni
A Consistent Model of the Accretion Shock Region in Classical T Tauri Stars
A Far-ultraviolet Atlas of Low-resolution Hubble Space Telescope Spectra of T Tauri Stars
A high-Resolution Catalog of Cometary Emission Lines
A new parallax measurement for the Pleiades star cluster
A Search for Low Mass Companions and a New Determination of Effective Temperature for T-Tauri Stars
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