Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
1=Centro de Radioastronomía y Astrofísica, UNAM, 2=Korea Astronomy and Space Science Institute, 3=Astrophysikalisches Institut Potsdam
Astrophysikalisches Institut Potsdam;
Heidelberg University, AIP
Zentrum fuer Astronomie der Universitaet Heidelberg
Inst. Theoretical Astrophysics Heidelberg
ITA Heidelberg
Emmy Noether Research Group at Astrophysical Institute Potsdam
Emmy Noether Group, AIP, Germany
Sterrewacht Leiden
1+2
Astrophysikalisches Institut Potsdam, Germany
Zentrum für Astronomie der Universität Heidelberg
ITA, University of Heidelberg, Germany
AIP, UC Santa Cruz
ITA, Heidelberg
Institut fuer Theoretische Astrophysik, Zentrum fuer Astronomie der Universitaet Heidelberg, Heidelberg, Germany
ITA-Heidelberg, Germany
Zentrum fuer Astronomie Heidelberg
Leiden Observatory, NL
MPI for Astronomy, Heidelberg
AIP, Potsdam
Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, Albert-Ueberle-Str. 2, 69120 Heidelberg, Germany
Institut für Theoretische Astrophysik, Universität Heidelberg, 69120 Heidelberg, Germany
Institut für Theoretische Astrophysik / Zentrum für Astronomie der Universität Heidelberg, Albert-Überle-Str. 2, D-69120, Germany für Astronomie der Universitát Heidelberg, Institut für theoretische Astrophysik, Albert-Ueberle Strasse 2, 69120 Heidelberg, Germany
Zentrum für Astronomie der Universität Heidelberg, Institute für theoretishe Astrophysik, Albert-Ueberle-Str. 2, 69120, Heidelberg
Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, Albert-Ueberle-Strasse 2, 69120 Heidelberg, Germany
Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, Albert-Ueberle-Str. 2, D-69120 Heidelberg, Germany; Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Menlo Park, CA 94025, USA
A Holistic Scenario of Turbulent Molecular Cloud Evolution and Control of the Star Formation Efficiency. First Tests
A new Jeans resolution criterion for (M)HD simulations of self-gravitating gas: Application to magnetic field amplification by gravity-driven turbulence
A quantification of the non-spherical geometry and accretion of collapsing cores
About the morphology of dwarf spheroidal galaxies and their dark matter content
Accretion-Driven Turbulence as Universal Process: Galaxies, Molecular Clouds, and Protostellar Disks
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