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  1. Magnetic Fields in Galaxies

    Magnetic fields are a major agent in the interstellar medium. They contribute significantly to the total pressure which balances the gas disk against...
    Rainer Beck in Cosmic Magnetic Fields
    Chapter
  2. Magnetic Fields in Galaxy Systems, Clusters and Beyond

    The discovery of significant magnetic fields beyond our Milky Way was unwittingly made in the early 1950’s when new “discrete” cosmic radio sources...
    Philipp P. Kronberg in Cosmic Magnetic Fields
    Chapter
  3. Stellar Magnetic Fields

    Stellar magnetic fields are directly detected or inferred across the whole Hertzsprung--Russell Diagram. Attention in this chapter is concentrated on...
    Leon Mestel, John D. Landstreet in Cosmic Magnetic Fields
    Chapter
  4. Magnetic Fields in Diffuse HI and Molecular Clouds

    The diffuse interstellar HI is the matrix within which many molecular clouds reside and the medium that soaks up the energy injected by sources such...
    C. Heiles, R. Crutcher in Cosmic Magnetic Fields
    Chapter
  5. Magnetic Fields in the Early Universe

    A substantial magnetic field could conceivably have been generated in the ultra-early Universe. However, the relevant physics at those eras is very...
    Martin J. Rees in Cosmic Magnetic Fields
    Chapter
  6. 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
  7. 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
  8. 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
  9. 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
  10. 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
  11. 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
  12. 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
  13. 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
  14. 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
  15. 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
  16. Introduction

    We summarize the topics presented in this book, and when appropriate we enlighten cross–references among the different topics: high precision and...
    Nora Bretón, Jorge L. Cervantes–Cota, Marcelo Salgado in The Early Universe and Observational Cosmology
    Chapter
  17. Cosmological Applications of Loop Quantum Gravity

    After a brief introduction to classical and quantum gravity we discuss applications of loop quantum gravity in the cosmological realm. This includes...
    Martin Bojowald, Hugo A. Morales-Técotl in The Early Universe and Observational Cosmology
    Chapter
  18. Quantum Corrections to Scalar Quintessence Potentials

    We give a brief introduction into the formalism of the effective action. We use the effective action to investigate the stability of scalar...
    Michael Doran, Joerg Jaeckel in The Early Universe and Observational Cosmology
    Chapter
  19. The Accelerating Universe and Dark Energy: Evidence from Type Ia Supernovae

    I discuss the use of Type Ia supernovae (SNe Ia) for cosmological distance determinations. Low-redshift SNe Ia (...
    Chapter
  20. Black Holes in Two Dimensions

    Models of black holes in (1 + 1)-dimensions provide a theoretical laboratory for the study of semi-classical effects of realistic black holes in...
    Yuri N. Obukhov, Friedrich W. Hehl in Black Holes: Theory and Observation
    Conference paper
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