Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
ASTRON, and Astronomical Institute, University of Amsterdam, The Netherlands
Amsterdam NL
ASTRON The Netherlands
Arizona University
Stichtung Radioastraling van zon en Melkweg, Dwingeloo, Netherlands
Stichting Radiostraling van Zon en Melkweg, Dwingeloo, Netherlands
NFRA, Dwingeloo, NL
Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA University, Tucson, Ariz.
Dwingeloo, Radiosterrenwacht, Netherlands
Netherlands Foundation for Radio Astronomy, Dwingelo.
Netherlands Foundation for Radio Astronomy, Dwingeloo, Netherlands
Radiosterrenwacht, Dwingeloo, Netherlands
ASTRON, Dwingeloo, Netherlands
Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA; of Planetary Sciences, Lunar and Planetary Laboratory, Tucson, AZ, USA; Radiosterrenwacht, Postbus 2, 7990 AA Dwingeloo, The Netherlands; and Astronomical Institute, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
Arizona, University, Tucson, AZ
Stichting Radiostralinaj van Zon en Milkweg, Dwingeloo, Netherlands
ASTRON, 7990 AA Dwingeloo, The Netherlands; Astronomical Institute 'A. Pannekoek', University of Amsterdam, 1098 SJ, The Netherlands
Leiden, Sterrewacht, Leiden, Netherlands
University of Arizona
ASTRON, Radiosterrenwacht, Postbus 2, 7990 AA Dwingeloo, The Netherlands; Astronomical Institute, University of Amsterdam, The Netherlands
Department of Planetary Sciences, Lunar and Planetary Laboratory, University of Arizona, 85721, Tucson, USA
Stichting Radiostraling van zon en Melkweg, Dwingeloo, Netherlands
Arizona Univ., Tucson.
Geological Survey, Flagstaff, AZ.
University of Southern California, Los Angeles.
Stichting Radiostraling van Zon in Melkweg, Dwingeloo, Netherlands
Stichting Radiostraling von Zon en Melkweg, Dwingeloo, Netherlands
Department of Planetary Sciences, University o
'Guest stars', sample completeness and the local supernova rate
1803 + 784 - A BL Lacertae object with remarkable radio properties
1919 + 742 - A large double radio source
1928 + 738 - A superluminal source with large-scale structure
1928+738: A Superluminal Source With Large Scale Structure
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