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Kolloquien und Seminare seit 2012

James W. Beletic (TELEDYNE Imaging Sensors, USA)
The Fantastical Discoveries of Astronomy made possible by the Wonderful Properties of II-VI Materials
Wolfgang Steffen (Instituto de Astronomica, UNAM, Ensenada, Mexico)
Astrophysical simulations with interactive computergraphi
Jaime Forero-Romero (Berkeley)
New topics in high-z galaxy formation
Jason Nordhaus (Rochester Institute of Technology)
Recent Advances in Core-Collapse Supernova Theory
Eberhard Wiehr (Göttingen)
Line Profiles of Ionized and Neutral Helium in Solar Prominences
Javiera Guedes (ETH Zürich)
The Eris Simulation: Forming Realistic Milky Way-like Galaxies Through Cosmological Simulations
Abhijit Bendre (AIP)
Simulations of supernova-driven galactic turbulence
Günther Rüdiger / Manfred Küker (AIP)
The Cross Helicity at the Solar Surface by Simulations and Observations
Elmo Tempel (Tartu Observatory, Estonia)
Orientation of galaxies in filaments: 3D photometrical modelling of galaxies and filamentary structure in the SDSS
Enn Saar (Tartu Observatory, Estonia)
Shadows of Baryonic Oscillations
Hongqi Zhang (Beijing, China)
Helicity from Solar Observations
Luigi Guzzo (INAF-OAB, Italy)
Understanding Cosmic Acceleration with Galaxy Redshift Surveys
Sladjana Nikolic (MPIA Heidelberg)
Supernova in 3D: VIMOS IFU observations of SN 1006
Michael Kramer (MPIfR Bonn)
Fundamental physics with radio astronomy
Pirin Erdogdu (UCL, London)
The 2MASS Redshift Survey: Reconstructed Density and Velocity Fields and the Local Group Dipole
Tanya Urrutia (AIP)
Feedback in action in luminous, young, dust-reddened QSOs
Andreas Faltenbacher (Cape Town)
Anisotropy in the matter distribution at very large scales
Benedetta Ciardi (MPA Garching)
Cosmic reionization: theoretical modelling and challenging observations
Stefano Ansoldi (Udine University)
A statistical approach to the determination of model parameters in astrophysics: The case of active galactic nuclei synchrotron-self compton models
Juan Carlos Munoz-Cuartas (AIP)
Properties of the distribution of dark matter

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