Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
Scientist
University of Oxford, U.K.
Caltech
California Institute of Technology
U. of Durham; Caltech
Mail Code 350-17, California Institute of Technology, 1200 E California Blvd, Pasadena, CA 91125, USA
California Institute of Technology, MC 105-24, Pasadena, California 91125
Department of Astrophysics, University of Oxford, Keble Road, Oxford OX1 3RH, UK
Mail Code 130-33, California Institute of Technology, Pasadena, CA 91125, USA
Durham
University of Oxford, UK
California Institute of Technology, U.S.A
University of Durham
University of Durham, Durham, UK
Dept. of Physics, Oxford
Theoretical Astrophysics, Caltech, Pasadena, U.S.A
California Institute of Technology, Pasadena, U.S.A
University of Durham, UK
Caltech, USA
Department of Astrophysics, University of Oxford, Keble Road, Oxford, UK
California Institute of Technology, USA
The California Institute of Technology
Theoretical Astrophysics, Caltech, 1200 E. California Blvd., Pasadena, CA 91125, USA; Kavli Institute of Theoretical Physics, Santa Barbara, CA 93106, USA
USNO
U.S. Naval Observatory, Flagstaff Station
Wyoming, University, Laramie
US Naval Observatory Flagstaff Station
U.S. Naval Obs.
Wyoming Univ., Laramie.
USNO, Flagstaff Station
US Naval Obs.
USNO Astrometry Dept.
Navy Prototype Optical Interferometer, US Naval Observatory, Flagstaff, AZ 86002-1149 Naval Observatory, USA
US Naval Observatory, Flagstaff Station, P.O. Box 1149, Flagstaff, AZ 86002-1149 Infrared Observatory, Laramie
US Naval Observatory, Flagstaff Station, P.O. Box 1149, Flagstaff, AZ 86002 Naval Observatory, Flagstaff, AZ 86002-1149
10 AU scale halo structure around DG Tauri
10 micron speckle interferometry observations of evolved stars
10 Micron Speckle Observations of Evolved Stars
A Comparison of Semi-Analytic and Smoothed Particle Hydrodynamics Galaxy Formation
A Comparison of Theoretical Models of Galaxy Evolution: Consequences for High Redshift Star Formation
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