Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Caltech
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
Department of Astronomy, California Institute of Technology, MC 105-24, 1200 East California Boulevard, Pasadena, CA 91125
MPE
Division of Physics, Mathematics and Astronomy, California Institute of Technology, Pasadena, CA.
University of Washington, ESS, Box 351310, Seattle, WA 98195, USA University, England
Washington, University, Seattle, WA; Texas A&M University, College Station, TX
Southampton, University, Southampton, England
Earth and Space Sciences; and Center for Astrobiology & Early Evolution, University of Washington Box 351310, Seattle, WA 98195, USA für extraterrestrische Physik, Germany
MPE, Germany
Southampton University, Southampton, England
Geophysics Program, University of Washington, Box 351650, Seattle, USA
Washington, University, Seattle
Washington Univ., Seattle
Department of Astronomy, Caltech
CfA
University of Washington, Seattle, Earth and Space Sciences 070 Johnson Hall 351310, Seattle, WA 98195, USA Time and Frequency Div., Boulder, CO
University of Washington, Department of Earth and Space Sciences, Box 351310 University of Washington, Seattle, WA 98195-1310, USA Department, Williams College, Williamstown, Massachusetts 01267
Rice University, Houston, Tex.
Oxford University, Oxford, England
Harvard-Smithsonian Center for Astrophysics
Swarthmore College, Swarthmore, PA 19081, USA
Department of Earth and Space Sciences, University of Washington, Box 351310, Seattle, WA 98195, USA University, Australia
NOAO
Princeton University
Oberlin College, Department of Physics and Astronomy 110 N. Professor St., Oberlin, OH 44074, USA Environment Research
17OH spin-rotation transition frequencies (Polehampton+, 2003)
A 30 AU radius CO gas hole in the disk around the Herbig Ae star Oph IRS 48
A deep optical/near-infrared catalog of Serpens
A Large Millimeter Flare on the RS CVn Binary σ Geminorum
A Measurement of the J = 2 1 Fine-Structure Interval for 28Si and 29Si in the Ground 3P State
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