Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Max Planck Inst. für Radioastronomie, Bonn, Germany für Radioastronomie, Bonn, Germany, and I. Physikalisches Institut, Universität zu Köln, Germany
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
I. Physikalisches Institut, Universität zu Köln, Zülpicher Strasse 77, 50937 Cologne, Germany
Max-Planck-Institut für Radioastronomie, Bonn, Germany; I. Physikalisches Institut, Universität zu Köln, Germany
Max-Planck-Institut für Radioastronomie
I. Physikalisches Institut, Universität zu Köln, Germany and Max-Planck-Institut für Radioastronomie, Bonn, Germany
MPIfR
Max Planck Insitut fuer Radioastronomie
KOSMA, Germany
Physikalisches Institut, Universitaet zu Koeln, Köln, Germany
I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937, Köln, Germany
Max-Planck-Institut für Radioastronomie, Auf dem Huegel 69, 53121 Bonn, Germany
Universität zu Köln, I. Physikalisches Institut, Zülpicher Str. 77, 50937 Köln, Germany
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA; Division of Engineering and Applied Sciences, Harvard University, Pierce Hall, 29 Oxford Street, Cambridge, MA 02138, USA
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138 and Division of Engineering and Applied Sciences, Harvard University, Cambridge, Massachusetts 02138
I. Physikalisches Institut, Universität zu Köln, Zülpicherstrasse 77, 50937 Cologne, Germany
I. Physikalisches Institut, Universität zu Köln, Zülpicher Str. 77, 50937 Köln, Germany
I. Physikalisches Institut, Universität zu Köln, Zülpicherstrasse 77, 50937 Cologne, Germany; Department of Engineering and Applied Sciences, Harvard University, Pierce Hall, 29 Oxford St., MA 02138, USA
I. Physikalisches Institut, Uni
A 12mm Line Survey Towards Sites of Massive Star Formation
A 3mm Line Survey Towards Sites of Massive Star Formation
A Concise New Look at the l-Type Spectrum of H12C14N
A detailed line survey of G327.3-0.6
A multi-transition submillimeter water maser study of evolved stars - detection of a new line near 475 GHz
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