Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Munich
Mount Wilson and Las Campanas Observatoires, Pasadena, CA
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, Postfach 1317, D-85741 Garching bei München, Germany
Mount Wilson and Las Campanas Observatoires, Pasadena, Calif.
Max-Planck-Institut für Physik und Astrophysik, Garching bei München, Germany
Cambridge University, Cambridge, England
ESO Scientific Group in Geneva
Hale Observatoires, Pasadena, Calif.
Max-Planck-Institut für extraterrestrische Physik, Garching bei München, Germany
Max-Planck-Institut für Physik und Astrophysik, Munich, Germany
Max-Planck-Institut für Physik und Astrophysik, 8046 Garching near Munich, Germany
Max-Planck-Institut für Astrophysik, Karl Schwarzscild-Str. 1, D-85740 Garching bei München, Germany
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; Kitt Peak National Observatory, Tucson, AZ
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; European Southern Observatory, Garching bei München, Germany; Edinburgh, University, Edinburgh, Scotland
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; Edinburgh, University, Edinburgh, Scotland; European Southern Observatory, Garching bei München, Germany
Max-Planck-Institut für Astrophysik
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; Arecibo Observatory, Arecibo, PR; European Southern Observatory, Garching bei München, Germany
Max-Planck-Institut für Astrophysik, 85741 Garching bei München, Germany
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; European Southern Observatory, Garching bei München, Germany
MPIfA, Germany
Mount Wilson and Las Campanas Observatoires, Pasadena, CA; Max-Planck-Institut für Astrophysik, Garching bei München, Germany
Mount Wilson Observatory, Pasadena, CA.
Max-Planck
21-cm observations of galaxies in groups and multiplets
3C 120 and the surrounding region of sky
3C 273 in perspective.
A BL Lacertae object near the spiral galaxy NGC 6503
A Cluster of High Redshift Quasars with Apparent Diameter 2.3 Degrees
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