Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Univ. Oregon
U. of Oregon
University of Oregon
Washington, University, Seattle, Wash.
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Palomar Observatory, Pasadena, CA; Kitt Peak National Observatory, Tucson, AZ; Arecibo Observatory, Arecibo, PR
California Institute of Technology, Pasadena
California Institute of Technology, Pasadena.
Palomar Observatory, Pasadena, CA
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
California Institute of Technology, Pasadena, CA; Kitt Peak National Observatory, Tucson, AZ
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
Department of Physics, University of Oregon, Eugene, Oregon 97403, USA
Smithsonian Astrophysical Observatory, Cambridge, MA.
Oregon Univ., Eugene.
Michigan, University, Ann Arbor
U Oregon
California Institute of Technology, Pasadena, CA; Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Kitt Peak National Observatory, Tucson, AZ
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; California Institute of Technology, Pasadena, CA; Observatorio Interamericano de Cerro Tololo, La Serena, Chile; National Astronomy and Ionosphere Center, Ithaca, NY
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; California Institute of Technology, Pasadena, CA; Kitt Peak National Observatory, Tucson, AZ
Oregon, University, Eugene
Department of Physics, University of Oregon, Eugene, OR 97403 of Arizona, Tucson, AZ
Palomar Observatory, Pasadena, CA; Arecibo Observatory, Arecibo, PR
Department of Physics, University of Oregon, 120 Willamette Hall, Eugene, OR 97403
California Institute of Technology, Pasadena, CA
Department of Physics and Astronomy, University of Oregon
0351+026 - A QSO spawned by interacting galaxies
1E 1415.6+2557 - an X-ray-selected BL Lacertae object in a luminous galaxy
21-cm Study of Over 100 Newly Discovered, Nearby LSB Galaxies
A catalog of radio, optical, and infrared observations of spiral galaxies in clusters
A constraint on the infall of H I into big disk galaxies
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