Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Cosmology and Extragalactic Astrophysics
Scientist
University of Alabama
Alabama, University, University, Ala.
Alabama, University, Tuscaloosa, AL
University of Alabama, Tuscaloosa
Cambridge University, England
University of Alabama, Department of Physics and Astronomy, P. O. Box 1921, Tuscaloosa, Alabama 35487
Tuorla Observatory University of Turku 21500 Turku Finland
Alabama, University, University, AL
Alabama, University, Huntsville, Ala.
Department of Physics and Astronomy, University of Alabama
University of Alabama, Tuscaloosa, AL, 35487-0324, USA
Alabama Univ., Tuscaloosa.
Department of Physics and Astronomy, University of Alabama, Box 870324, Tuscaloosa, AL 35847
University of Alabama, Tuscaloosa, AL 35487-0324, USA
University of Alabama, Tuscaloosa, USA
University of Alabama, Tuscaloosa, AL
University of AL
Alabama University
Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487-0324
University of Alabama, PO Box 870324, Tuscaloosa, Alabama 35487-0324
Los Alamos National Lab., NM.
Alabama Univ., Huntsville.
Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487
Department of Physics and Astronomy, University of Alabama, Tuscaloosa, Alabama 35487, USA
Alabama Univ., Tuscaloosa, AL
NASA, Marshall Space Flight Center, Huntsville; Alabama, University, Tuscaloosa, AL
Department of Physics, and Astronomy Department, University of Alabama, Tuscaloosa, AL 35487.
Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487, USA
Department of Physics and Astronomy, University of Alabam
A binary model for the Coma cluster of galaxies
A Computer Model of the Origin of H i Radial Velocity Asymmetries in M31
A Hubble Space Telescope Optical and Ground-based Near-Infrared Study of the Giant Nuclear Ring in ESO 565-11
A Hubble Space Telescope Study of Star Formation in the Inner Resonance Ring of NGC 3081
A method for determining the beam geometry of SS 433 using high-resolution radio observations
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