People

PhD Students

Daniel Karner


phone:   

email:   dkarner[at]usm.lmu.de

office:   USM 006




Processes for generating cosmic rays and magnetic fields in galaxy clusters

 Laura Di Federico

phone:   

email:   laudif[at]usm.lmu.de

office:   USM 5A




Cooling processes in Galaxy and Galaxy Cluster Formation

Silvio Fortuné


phone:   

email:   sfortune[at]usm.lmu.de

office:   USM




Spin Evolution in Galaxies


Energy balance in cool core galaxy clusters: The interplay of gravitational collapse and AGN feedback in a cosmological background

Justo Gonzalez

 
phone:  

email:   justoagv[at]gmail.com

office:   ESO




Impact of the Hydrodynamical Scheme on Simulations of Galaxies & Galaxy Clusters

Frederick Groth

 
phone:  

email:   fgroth[at]usm.lmu.de

office:   USM




Local Universe Simulations 

Elena Hernández Martínez

 
phone:  

email:   hernandez[at]usm.lmu.de

office:   USM





Galaxy Evolution in Cluster Environments

Anna Ivleva

 
phone:  

email:  ivleva[at]usm.lmu.de

office:   USM 006

Lucas Kimmig


phone:   

email:   lkimmig[at]usm.lmu.de

office:   USM


  • Structure Formation and Evolution from Galaxies to Galaxy Clusters
  • Hydrodynamical Simulations
  • Galaxy Cluster Properties



The Kelvin-Helmholtz Instability: 

Eulerian hydrodynamics vs numerical dissipation 

Tirso Marin

 
phone:  

email:   tmarin[at]usm.lmu.de

office:   USM





The origin and evolution of large scale filaments in local galaxies

Hans-Christian Poosch

 
phone:  

email:  hans.poosch[at]
            campus.lmu.de

office:   MPE X2/364


Hans-Christian Poosch

 
phone:  

email:  hans.poosch[at]
            campus.lmu.de

office:   MPE X2/364


Leonard Romano

phone:  +49 89 30000 3884 

email:   lromano[at]usm.lmu.de

office:   MPE X2/364

publications, GitHub



Turbulence in Galaxies, Local Bubble



Voids in the Magneticum Simulation

Benjamin Seidel


phone:  +49 89 30000 3884 

email:   bseidel[at]usm.lmu.de

office:   USM




Spectral Analysis of Star-Forming Galaxies with traditional and machine learning methods

Eva Sextl

 
phone:  

email:   eva.sextl[at]campus.lmu.de

office:   USM 110 (I 16)



- Origin of Magnetic Fields and Multi Messenger Particles in the Local Universe

- Chemodynamical Properties of simulated Galaxies

Johannes Stoiber

 
phone:  

email:   jstoiber[at]usm.lmu.de

office:   USM 006




- Primordial black holes

- Turbulence in the ISM

Valentin Thoss

 
phone:  

email:   

office:   MPE X2/364




- Kinematics of galaxies in cosmological simulations 

- Kinematic tracer populations: globular clusters & planetary nebulae

Lucas Valenzuela


phone:   

email:   lval[at]usm.lmu.de

office:   USM



Galactic X-ray scaling relations and cosmic X-ray background

Stephan Vladutescu-Zopp

 
phone:  

email:   vladutescu[at]usm.lmu.de

office:   USM


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