Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Padova, Un.
Astr.Dept., Padova
25,+
MPI fuer Astrophysik
MPA-Garching
MPA-GARCHING
Max-Planck-Institut fur Astrophysik - Garching
MPA, Garching
MPA Garching
Max-Planck-Institut für Astrophysik Garching
Universita' di Padova
Max-Planck-Institut für Astrophysik, Garching b. München, Germany
Dipartimento di Astronomia, Università di Padova, Italy
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild Strasse 1, Garching bei München, Germany
Max Planck Institute for Astrophysics, Germany
MPI for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching bei München, Germany
Dipartimento di Astronomia, Università di Padova Vicolo dell'Osservatorio 2, 35122 Padova, Italy
Max-Planck-Institut für Astrophysik, PO Box 1317, 85741 Garching bei München, Germany
Dipartimento di Astronomia, Università di Padova, Vicolo dell'Osservatorio 2, 35120 Padova, Italy; Max-Planck-Institut für Teoretische Astrophysik, 85748 Garching bei München, Germany
Max-Planck-Institut für Astrophysik, P.O. Box 1317, 85741 Garching bei München, Germany
MPI for Astrophysics Garching
University Observatory, Munich
Max Planck Institute for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching, Germany
Dipartimento di Astronomia, Università di Padova, vicolo dell'Osservatorio 5, 35122 Padova, Italy
Dipartimento di Astronomia, Università di Padova, Padova, Italy
MPI for Astrophysic, Karl-Schwarzchild-Str. 1, D-85741 Garching bei München, Germany
MPI for Astrophysics, Karl-Schwarzschild-Str. 1, D-85741 Garching bei München, Germany for Astrophysics, Karl-Schwarzchild-Str. 1, D-85741 Garching bei München, Germany
A Comparison of Cosmological Codes: Properties of Thermal Gas and Shock Waves in Large Scale Structures
A fast method for computing strong-lensing cross sections: Application to merging clusters
A full sky prediction of the SZ effect from diffuse hot gas in the local universe and the upper limit from the WMAP data
A new Monte Carlo Generator for Ultra-High Energy Cosmic Rays from the Local and Distant Universe
A non-ideal MHD Gadget: Simulating massive galaxy clusters
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