Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Galaxy Astrophysics
Scientist
KUL
U. Leuven
Instituut voor Sterrenkunde, K. U. Leuven, Belgium
Instituut voor Sterrenkunde, Leuven, Belgium
IvS
Instituut voor Sterrenkunde, K.U. Leuven, Celestijnenlaan 200 B, 3001 Leuven, Belgium
Instituut voor Sterrenkunde, Celestijnenlaan 200D, 3001 Leuven, Belgium
Department of Physics and Astronomy, Institute of Astronomy, University of Leuven, Celestijnenlaan 200D, 3001 Heverlee, Belgium
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200D, 3001, Leuven, Belgium; Sterrenkundig Instituut Anton Pannekoek, University of Amsterdam, Science Park 904, 1098, Amsterdam, The Netherlands
Department of Physics and Astronomy, Institute for Astronomy, K.U. Leuven, K.U. Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
Instituut voor Sterrenkunde, Department of Physics and Astronomy, K.U. Leuven, Celestijnenlaan 200D, 3001, Leuven, Belgium; Sterrenkundig Instituut Anton Pannekoek, University of Amsterdam, Kruislaan, 403 1098, Amsterdam, The Netherlands;
Department of Physics and Astronomy, Institute for Astronomy, K. U. Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium for Sterrenkunde, Katholieke Universiteit Leuven, Belgium
Catholique University of Leuven Department of Physics and Astronomy of Physics and Astronomy, Institute of Astronomy, K.U. Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium ; Sterrenkundig Instituut Anton Pannekoek, University of Amsterdam, Kruislaan 4031098 Amsterdam, The Netherlands voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001 Heverlee, Belgium
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, B-3001 Heverlee, Belgium
KU Leuven, Belgium
Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
Instituut voor Sterrenkunde, K.U.Leuven, Celestijnenlaan 200B, 3001 Leuven, Belgium
Instituut voor Sterrenkunde, Katholieke Universiteit Le
A chemical inventory of the S-type AGB star χ Cygni based on Herschel/HIFI observations of circumstellar line emission. The importance of non-LTE chemical processes in a dynamical region
A far-infrared survey of bow shocks and detached shells around AGB stars and red supergiants
A HIFI preview of warm molecular gas around chi Cyg : first detection of H2O emission toward an S-type AGB star
A high resolution line survey of IRC+10216 with Herschel. First results: Detection of warm silicon dicarbide SiC2
A Spitzer Sample of S-type AGB Stars
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