Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
MPIK, Germany
Astrophysics Division, Max-Planck-Institut für Kernphysik
MPIK, Heidelberg
MPIK, Heidelberg, Germany
Max-Planck-Inst. für Radioastronomie, Bonn, Germany
Paris VII Univ., France
Max-Planck-Institut für Kernphysik, 69029 Heidelberg, Germany
Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany
Max-Planck-Institut für Kernphysik, Heidelberg, Germany
Max-Planck-Institut für Kernphysik, Astrophysics Department
Max Planck Institut
Mullard Radio Astronomy Observatory, Cambridge, England
Max-Planck-Institut für Kernphysik, Heidelberg
MPI-Kernphysik, Heidelberg, Germany
Astronomiska observatoiret, Uppsala, Sweden
Max-Planck-Institut für Kernphysik, Postfach 10 39 80, 69029 Heidelberg, Germany
Max-Planck-Institut für Kernphysik, Saupfercheckweg, D-69117 Heidelberg, Germany
Max-Planck-Institut für Radioastronomie, Bonn, Germany
MPI für Kernphysik, Postfach 103980, D--69117 Heidelberg, Germany
MPIK Heidelberg
MPIK Heidelberg, Germany;
Max Planck Institut fuer Kernphysik, Heidelberg;
Max Planck Institut fuer Kernphysik, Astrophysics Department, Heidelberg, Germany
Astrophysics Division, Max-Planck-Institut fuer Kernphysik
Max-Planck-Institute for Nuclear Physics Heidelberg
Max-Planck-Institut für Kernphysik, Astrophysics Department, Saupfercheckweg 1, D-69117 Heidelberg, Germany
Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany
Max-Planck-Institut für Kernphysik, Germany
Max-Planck-Institut für Kernphysik, Astrophysics Department, Saupfercheckweg 1, 69117 Heidelberg, Germany
Max Planck Institut fuer Kernphysik, Heidelberg
A comparative study of the spatial distribution of ultraviolet and far-infrared fluxes from M 101
A Comparative Study of the Spatial Distribution of Ultraviolet and Far-infrared Fluxes from M101
A comparative study of the spatial distribution of ultraviolet and far-infrared fluxes from M101.
A GALEX-ISOPHOT Resolved Study of M101
A linear near-IR Tully-Fisher relation for giant and dwarf late-type galaxies
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