Galactic Evolution and Stellar Dynamics

Staff

Prof. Dr. Gerhard Hensler

e-mail : supas030@astrophysik.uni-kiel.de
Tel. : +49-431-880-4125

Dr. Joachim Köppen

e-mail : supas086@astrophysik.uni-kiel.de
Tel. : +49-431-880-4103

Dr. Christian Theis

e-mail : supas033@astrophysik.uni-kiel.de
Tel. : +49-431-880-1574

Dipl.-Phys. Tim Freyer

e-mail : supas055@astrophysik.uni-kiel.de
Tel. : +49-431-880-4101

Dipl.-Phys. Andreas Rieschick

e-mail : supas039@astrophysik.uni-kiel.de
Tel. : +49-431-880-1575

Dipl.-Phys. Daniel Tschöke

e-mail : supas105@astrophysik.uni-kiel.de
Tel. : +49-431-880-1575

Dipl.-Phys. Wolfgang Vieser

e-mail : supas110@astrophysik.uni-kiel.de
Tel. : +49-431-880-4101

Stefan Harfst

e-mail : supas122@astrophysik.uni-kiel.de
Tel. : +49-431-880-3682

Lars Kleinschmidt

e-mail : kleinsch@astrophysik.uni-kiel.de
Tel. : +49-431-880-4060

Sören Kühnholz

e-mail : supas101@astrophysik.uni-kiel.de
Tel. : +49-431-880-4060

Jan-Uwe Ness

e-mail : supas103@astrophysik.uni-kiel.de
Tel. : +49-431-880-4119

Christian Neuerer

e-mail : cneuer@astrophysik.uni-kiel.de
Tel. : +49-431-880-3682

Tobias Rettstadt

e-mail : supas116@astrophysik.uni-kiel.de
Tel. : +49-431-880-4126

Hermann Timmen

e-mail : supas115@astrophysik.uni-kiel.de
Tel. : +49-431-880-3682

Projects

Interstellar Medium

• Dynamical Evolution of the Interstellar Medium
  • Dynamics of a Multiphase Gaseous Medium
  • Collisions of Interstellar Clouds
  • Superbubbles
  • Self-Regulation of Star Formation
• Non-Dynamical Evolution of the Interstellar Medium

Structure and Evolution of Galaxies

• Structure of the Milky Way
  • Metallicity Gradient of the Disk
  • Vertical Structure of the Disk
• Extragalactic Systems
  • Star Formation Rate in Spiral Galaxies
  • Multi-Wavelength Observations of Starburst-Galaxies
• Galactic Evolution
  • Evolution of Cloud Systems
  • Galactic Gas Dynamics
  • Chemo-Dynamics
• Stellar Dynamics
  • Anisotropy in Collapsing Systems
  • Shape Evolution
  • Softening and Relaxation
  • GRAPE-Project

Publications of the working group Hensler

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