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Topics chosen in the WS 12/13:
Topics of the 1st Semester:
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| Name | Topic | Date | Supervisor |
| 1. xx | Broad
and narrow lines regions in quasars. or Theory of the formation of Stroemgren spheres. |
Hoffmann | |
| 2. xx | The
orbital structure of galaxies. or Surface brightness profiles of elliptical galaxies. |
Thomas | |
| 3. xx | The wind-momentum luminosity relation. | Puls | |
| 4. xx | Imprints of Reionization on the Cosmic Microwave Background. | Weller | |
| 5. xx | The
spectral classification scheme. or The Stellar Initial Mass Function. |
Butler | |
| 6. xx |
Gas
and Dust in the Milky Way. or Gunn-Peterson effect. |
Gerhard | |
| 7. xx | The
gravitational lens effect.
or Are Elliptical Galaxies made by mergers? |
Seitz | |
| 8. xx | Formation mechanisms of high-mass stars. | Preibisch | |
| 9. xx | Hierarchy of instabilities in the Interstellar Medium. | Lesch | |
| 10. xx | The Evolution of Protoplanetary Disks | Ercolano | |
| Name | Topic | Date | Supervisor |
| 1. xx | Faraday Rotation (RM) of polarized radio emission. | ||
| 2. xx | Astrometry: Useful
since the times of Kepler. or c2 - fitting: Seeking the most likely truth. |
Gillessen | |
| 3. xx | Extra-solar
Planets: The various detection methods. or The Kepler Mission: Searching for a twin of the Earth. |
Koppenhoefer | |
| 4. xx | Measuring the large scale distribution of galaxies. | Phleps | |
| 5. xx | Adaptive
Optics: Correcting the atmospheric turbulence for ground- based
telescopes. or Modern eyes in astronomy - CCDs and IR detectors. |
Gillessen | |
| 6. xx | Detection of Gravitational Waves. | Ratzka | |
| 7. xx | Ritchey-Cretien-Telescopes (VLT, WST 2m, PanSTARRS): The impact of science on the optical design. | Grupp | |
| 8. xx | Hertzsprung-Russell diagram, Colour-Magnitude diagram and globular clusters. | Riffeser | |
| 9. xx | What can the content of galaxy clusters tell us about the dark matter density in the Universe? | Mohr | |
| 10. xx | Experimental
Methods of Infrared Astronomy: The Key to the Galactic Center. or Getting most out of your data - Data Reduction. |
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| Name | Topic | Date | Supervisor |
| 1. xx | Why
is the cosmic microwave background fluctuation level 10-5? or Clumping in hot star winds. |
Lesch | |
| 2. xx | The Formation of Planets. or Galaxy evolution: From z~3 to present day. |
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| 3. xx | Simulations
of gravitating particle systems: Evolution of star clusters and galaxies. or Type Ia supernovae in modern astrophysics. |
Naab | |
| 4. xx | Dynamical
modeling and the structure of elliptical galaxies: Dark matter and the
formation epoch of ellipticals. or Line broadening and other misdemeanours. |
Thomas | |
| 5. xx | Cosmological Simulations of Galaxy Clusters. | ||
| 6. xx | Measuring
Dark Matter with Strong Gravitational Lensing. or Weak gravitational lensing: strech & flex of galaxies. or Two Point Correlation Functions. |
Seitz | |
| 7. xx | Spherical
Collapse in a Dark Energy Dominated Universe. or Spectral Energy Distributions of the first Stars and the Reionization of the universe. |
Weller | |
| 8. xx | Galaxy Models with NMAGIC. or Dark matter and structure formation in the Universe? |
Gerhard | |
| 9. xx | Triggering of star formation. | Preibisch | |
| 10. xx | Explaining cosmic acceleration with Dark Energy. | Hoyle/Weller | |
| Name | Topic | Date | Supervisor |
| 1. xx | How does one make precise measurements of 1 billion galaxies? | Mohr | |
| 2. xx | VISIR: State-of-the-art instrumentation for thermal infrared studies. or Advanced image processing: Deriving fundamental properties of the Galactic Center Supermassive Black Hole and its stellar neighborhood. |
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| 3. xx | What have we learned in the field of star formation from Optical Long Baseline Interferometry. | Ratzka | |
| 4. xx | The
stellar structure of the Galaxy. or Intermediate-mass Black Holes. |
Phleps | |
| 5. xx | `Needles
in the Heystack' Searching for Machos and Planets with the difference imaging technique. |
Koppenhoefer | |
| 6. xx | Synthesizing
stellar isochrones to observed stellar populations. or Exploring telescope optics: How do the largest optical systems work? |
Riffeser | |
| 7. xx | Optical
Interferometry: Breaking the diffraction limit of individual telescopes. or Advanced Adaptive Optics: Laser Guide Stars and Multi-Conjugated Adaptive Optics. |
Gillessen/ Eisenhauer |
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| 8. xx | Adaptive
optics and laser guide stars: Compensating the atmospheric turbulence for diffraction limited images. or SINFONI: Spectro-Imaging and threedimensional data. |
Gillessen | |
| 9. xx | Astronomical CCD Cameras. | Lang | |
| 10. xx |
Probing the nature and
evolution of distant galaxies. or Detailed views of the era when stars have formed - the high-redshift Universe. |
Kurk | |
| Last updated April 2013 by A.W.A. Pauldrach uh10107@usm.lmu.de |