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  1. Searching the Trans-Neptunian Region

    The Edgeworth-Kuiper-Belt is considered to be the remnant of the formation disk of the planetary system around the Sun. For about 8 years the...
    Hermann Boehnhardt, Olivier R. Hainaut in Deep Fields
    Conference paper
  2. Course 15: Observations of the High Energy $\gamma$ -Ray Universe

    This article describes the nature and current status of observational programs studying astrophysical high energy...
    Conference paper
  3. Course 1: Accretion and Ejection-Related MHD

    This lecture is an introduction to MHD. Relevant equations, both in the classical and special-relativistic regimes are derived. The magnetic field...
    Conference paper
  4. Course 7: Cosmic Rays and Particle Acceleration at Astrophysical Shocks

    The acceleration of particles in the vicinity of astrophysical shocks has become the main paradigm in astrophysics for the production of cosmic rays...
    Conference paper
  5. Course 12: Evolution of YSO Disks

    As stars and planets form from accretion processes in disks, it is important to understand these processes and their evolutionary implications. While...
    Conference paper
  6. Course 11: Accretion Signatures in Young Stellar Objects

    Mass accretion onto the star is taken place in young stellar objects, providing the energy needed to power the excess emission observed at all...
    Conference paper
  7. Course 8: The Black Hole Environments

    Compact objects are astrophysical entities with radii smaller than about 10 Schwarzschild radii. The mass spectrum of these objects ranges from the...
    Conference paper
  8. Course 13: X-Rays from YSOS: Desperately Seeking the Central Engine

    The earliest stages of the evolution of low-mass stars are characterized by the presence of powerful jets, likely originating from accretion via...
    Conference paper
  9. Course 6: Gamma-Ray Bursts

    This lecture is an introduction to the study of gamma-ray bursts. Observations of the burst and its afterglow are first reviewed, with the...
    Conference paper
  10. Course 9: Accretion around Active Galactic Nuclei

    In bright AGN, at distances of several Schwarzschild radii, the accretion onto a black hole proceeds predominantly in a form of a cool accretion...
    Conference paper
  11. Laboratory Limits on Neutrino Masses

    The recent neutrino oscillation experiments have obtained nonzero differences of squared neutrino masses and therefore proven that neutrinos are...
    Christian Weinheimer in Neutrino Mass
    Chapter
  12. Experimental Results on Neutrino Oscillations

    Neutrino physics, in particular the question of neutrino mass and oscillations, is currently giving rise to a minirevolution in particle physics....
    Achim Geiser in Neutrino Mass
    Chapter
  13. Astrophysical and Cosmological Constraints on Neutrino Masses

    We review some astrophysical and cosmological properties and implications of neutrino masses and mixing angles. These include constraints based on...
    Kimmo Kainulainen, Keith A. Olive in Neutrino Mass
    Chapter
  14. Planet Formation

    Motivating the study of planet formation is not difficult for any curious audience. One of the fundamental human questions is that of origins: “where...
    Chapter
  15. Orbit Dynamics, Stability and Chaos in Planetary Systems

    Let us start with a problem of dynamical biology, which was posed about 800 years ago by Fibonacci1
    Rudolf Dvorak, Florian Freistetter in Chaos and Stability in Planetary Systems
    Chapter
  16. Velocity Dispersion Analysis of CNOC Clusters

    I present results of the analysis of the internal velocity dispersions,...
    Conference paper
  17. Magellanic Cloud Eclipsing Binaries: Distances and Dimensions

    In this contribution we analyse previously unpublished radial velocity curves in conjunction with other already published light curves, Strömgren...
    Conference paper
  18. The Galactic Bulge: Prospects for the VLT

    The central bulge of the Galaxy is 100 times closer than the nearest extragalactic bulge, that of M31. Until the era of 100m telescopes arrives, the...
    Conference paper
  19. The Stellar Mass Function

    Considerable progress has been made recently in more accurately determining the frequency distribution of stellar masses in the critical 0.1 to 1 m...
    Conference paper
  20. Extrasolar Planets Transits: Detection and Follow-Up

    The detection of transits has a rich potential of information about extrasolar planets. This contribution gives an overview and new perspectives on...
    Conference paper
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