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Alexander Arth
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Performing MHD simulations with Tree-PM/SPH Code Gadget. Implementing anisotropic conduction to improve simulations of galaxy cluster formation. |
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Jaime Abella Payá
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Simulations of clumps in z~2 galaxies with stellar feedback |
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Michael Aumer
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High-redshift galactic disk formation and structure |
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Alessandro Ballone
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Stellar winds in Galactic Nuclei; the galactic center cloud G2 |
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Eirini Batziou
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The Interplay of magnetic fields and and star formation processes in galaxies using SPMHD simulations. |
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Antonia Bevan
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Protoplanetary discs around young stars. |
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Adrian Bittner
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Disk galaxies in cosmological zoom-in simulations |
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Matias Blaña
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Stellar and galactic dynamics, Barred galaxies, Andromeda (M31), Dwarf spheroidal galaxies, Star clusters, N-body simulations, Made-to-measure modelling. |
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Max Brunner
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Self-regulated star formation in and evolution of galactic disks, including as infall from the cosmic web |
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Pawel Ciecielag
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Planets formation: planetesimals accretion, gas drag, disk-planet interaction; Cosmology: large scale velocity fields, density-velocity comparisions; Numerical methods: direct n-body (Nbody4++ code, special purpose hardware - GRAPE), hydro (PPM, AMR, FLASH code). |
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James Dale
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3-D SPH simulations of the effects of stellar feedback, particularly photionization and stellar winds, on star-forming molecular clouds, to investigate the likelihood of triggered star formation and to evaluate the disruptive effect of feedback on embedded clusters. |
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Clare Dobbs
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Molecular cloud formation in spiral galaxies. Formation of spiral galaxies. |
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Elena D'Onghia
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Galaxy and Structure Formation, the nature of dark matter, galaxy evolution, groups of galaxies. |
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Julius Donnert
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On the non-thermal emission in galaxy clusters
Supervisors: Klaus Dolag, Harald Lesch |
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Franziska Eisner
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Differences between observations and simulations of metallicities in galaxies |
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Bernat Ferrer
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Michael Kastl
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Katharina Fierlinger
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Interaction of massive star groups with the ISM: hydro models for radioactive tracers in the Orion Eridanus Superbubble. Codes: RAMSES |
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Pascal Förster
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Satellite galaxies in large-scale cosmological simulations; Turbulence in SPH |
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Michael Frühauf
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Asteroids, Near-Earth Objects, Impact Avoidance |
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Wolfgang von Glasow
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Galactic Winds: launching galactic outflows and feedback processes |
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Matthias Gritschneder
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Photoionisation in the environment of young, massive stars. Study of triggered star formation in proximity to these efficient ionisation sources. Numerical methods: SPH + Ionisation, VINE. |
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Bendix Hagedorn
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Evolution and dynamics of cold gas in simulated galaxies |
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Sebastian Hammer
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Simulations of collisions between gas clouds and disk galaxies
|
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Helmut Hetznecker
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Large scale structure formation, structure of dark matter halos, dwarf galaxies in dark matter halos |
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Michael Hilz
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Binary black hole mergers in galaxies (VINE code) |
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Paul Hinz
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Update of the GADGET Code with a new Meshless Finite Mass (MFM) algorithm for the hydrodynamics and testing of the implications on structure formation |
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Michaela Hirschmann
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Origin of the anti-hierarchical growth of black holes in the universe |
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David Hubber
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Developing the Graphical Astrophysics code for N-body Dynamics And Lagrangian Fluids (GANDALF) primarily designed for investigating star formation and planet formation. |
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Francesca Iannuzzi
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Studying the survival of galaxies in hydrodynamical simulations of clusters
Supervisors: Klaus Dolag, Simon White |
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Martin Ilgner
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Photoionisation models of the ISM, Chemistry and dynamics of protoplanetary discs |
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Roland Jesseit
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Orbital theory, stellar dynamics, galaxy formation, physics of dark matter halos. |
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Peter Johansson
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Galaxy and structure formation, analytic and numerical modelling of feedback, modelling of galaxy populations. |
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Veronika Junk
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Formation and dynamics of galaxy substructure; problem of the missing satellites. |
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Simon Karl
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Galaxy mergers with respect to the growth of central black holes (VINE code) |
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Geray Karademir
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Cosmological zoom-in simulations with a focus on galaxy groups |
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Madhura Killedar
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Testing galaxy cluster mass measurement techniques with numerical simulations and triaxial mass models, weak and strong gravitational lensing, cosmology, Bayesian inference and regression methods |
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Manuel Ködel
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HI-Gas dynamics of galaxies and galaxy clusters in the cosmological simulation Magneticum
|
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Christine Maria Koepferl
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Protoplanetary discs around young stars. |
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Hanna Kotarba
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With Prof. Harald Lesch: Magnetic field evolution in isolated and interacting spiral galaxies. Numerical methods: N-body/SPH (GADGET) |
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Martin Krause
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Radiation hydrodynamics at opacity transitions; Energy transport in molecular tori. The role of activity in galaxy evolution, multiphase turbulence, astrophysical jets, magnetic fields in galaxy clusters (SKADS) |
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Maximillian Kühn |
Kinematics of BCG's in cool core and non-cool core clusters |
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Bernd Lang
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Formation of stars, Turbulence, Accretion Disks, Prestellar Cores and Molecular Clouds, Radiative Transfer. |
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Guang-Xing Li
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Connecting theoretical and observational star formation study. Studying the structure of molecular clouds using the G-viral method. |
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Marcel Lotz
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Anisotropies in galaxy clusters |
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Chiara Mastropietro
|
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Emilio Mevius
|
Metallicity in cosmological simulations |
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Georg Michna
|
TBD |
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Nickolas Moeckel
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Hydrodynamics and stellar dynamics of young star clusters and star forming regions. The interplay between stellar and planetary dynamics. |
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Birgitta Müller
|
The Structure of Cold Dark Matter Halos |
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Thorsten Naab
|
|
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Judith Ngoumou
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Massive star feedback and triggered star formation |
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Eva Ntormousi
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Molecular cloud formation in colliding flows |
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Ludwig Oser
|
The formation of the Hubble Sequence (GADGET code) |
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Go Ogiya
|
Dynamical structure of dark matter halos, Small-scale problems of cold dark matter cosmology, GPGPU |
|
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Beata Pasternak
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Non-thermal emission from galaxy clusters - evolution of cosmic rays in merging galaxy clusters.
|
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Stephanie Pekruhl
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with Prof. Th. Preibisch: Observations & Simulations of Molecular Cloud Structure |
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Antonio Ragagnin
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Cosmological Simulations |
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Daniel Rahner
|
Formation of fast rotating elliptical galaxies by multiple minor mergers. |
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Lennart Reb
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Modelling the Spectral Energy Distribution of Low Luminosity Active Galactic Nuclei |
|
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Francesco Rizzuto
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Empirical galaxy formation models with warm dark matter |
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Giovanni Rosotti
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SPH simulations of accretion disc, both protoplanetary discs, to evaluate the effect of X-ray photoionization on the evolution of the disc, and discs around supermassive black holes. |
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Marc Schartmann
|
Hydrodynamical and radiative transfer simulations of (Active) Galactic Nuclei |
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Anna Schauer
|
Planetary Nebulae as tracers in Elliptical Galaxies |
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David Schlachtberger
|
The Origin of Cold Gas in Elliptical Galaxies: Zoom-in Simulations with Gadget3 |
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Philipp Schneider
|
Early phases of star formation - velocity and density structure of filaments in turbulent molecular clouds. |
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Felix Schulze
|
Kinematics of early type galaxies in cosmological simulations. |
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Florian Semrau
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Federico Stasyszyn
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Smoothed particle magneto-hydro-dynamics for cosmological applications
Supervisors: Klaus Dolag, Simon White |
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Lisa Steinborn
|
Active Galactic Nuclei in cosmological simulations |
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Ulrich Steinwandel
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Galaxy formation at high-redshift, supernova feedback, formation of black holes |
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Jens Stücker
|
Investigation of structure formation with warm dark matter in high resolution simulations |
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Stefanie Walch
|
Star formation with emphasis on the formation of protostellar disks, evolution and fragmentation of protoplanetary disks and the evolution of their spectral energy distributions. Numerical Methods: Grid-AMR: FLASH code; SPH: VINE code |
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Markus Wetzstein
|
Galaxy interactions / mergers, structure formation in the tidal arms of merging galaxies, formation of tidal dwarf galaxies, numerical methods for N-body / SPH (smoothed particle hydrodynamics) simulations, the VINE simulation code, special purpose hardware GRAPE for the computation of gravitational forces, implementation of the SPH algorithm on an FPGA (field programmable gate array) based special purpose hardware. |
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Martin Zintl
|
SPH simulations with GPU |
