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Recent Seminars

20 Oct 2015 - 10:30
Neil Vaytet
StarPlan
Stars form within turbulent complexes scaling hundreds of parsecs, harboring thousands of solar masses of cold gas: the...
28 Sep 2015 - 14:00
Adwin Boogert
USRA-Stratospheric Observatory for Infrared Astronomy, NASA Ames, USA
Freeze-out of the gas phase elements onto cold grains in dense interstellar and circumstellar media builds up ice...
15 Sep 2015 - 14:00
Yuri Fujii
Niels Bohr International Academy / StarPlan
The magnetorotational instability (MRI) is important for the dynamical evolution of protoplanetary disks through...
07 Sep 2015 - 14:00
David John Williamson
Laval University, Quebec, Canada
We have performed a series of "chemodynamic" simulations of isolated dwarf disc galaxies to determine how metals escape...
30 Jul 2015 - 14:00
Holly Capelo
Max Planck Institute for Dynamics and Self-Organization, Göttingen, Germany
It remains to be explained how kilometer-sized planetary embryos form from millimeter-sized particles in the dust-laden...
28 Jul 2015 - 14:00
Pedro Capelo
Institute for Computational Science, University of Zürich, Switzerland
I present the latest results from a suite of high-resolution hydrodynamical simulations of mergers between two late-...
16 Jun 2015 - 13:15
Erik Høg
Niels Bohr Institute, University of Copenhagen
The importance of discovering thousands of long-period exoplanets with up to 40 years period seems obvious. This can...
11 Jun 2015 - 14:00
Rosina Hein Bertelsen
Kapteyn Institute, University of Groningen
In protoplanetary discs dynamical effects due to planet formation are expected to lead to a gradual removal of material...
04 May 2015 - 14:00
Joanna Drążkowska
Institute for Computational Science, University of Zürich, Switzerland
There are almost 2000 known exoplanets and indirect methods indicate that every star in our Galaxy has on average more...
29 Apr 2015 - 14:00
Mihkel Kama
Leiden Observatory, The Netherlands
Carbon is a key element in the chemistry of protoplanetary material, and the backbone of life. The abundance of carbon...

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