Formato de una charla: Seminario

  • Charla
    Structure of the Kerr-Schild geometry, beam-like solutions and fluctuations of the black-hole horizon
    Exact solutions of the Einstein-Maxwell equations in the Kerr-Schild formalism are discussed. We show that black hole horizon is unstable with respect to...
  • Charla
    Study of molecular clouds associated with HII regions
    The properties of molecular clouds associated with 10 H II regions were studied using CO observations. We identified 142 dense clumps within our sample and...
  • Charla
    Study of the diversity of AGN dust models
    The dust component of active galactic nuclei (AGN) produces a broad infrared spectral energy distribution (SED), whose power and shape depends on the fraction...
  • Charla
    Study of the planetary system HD 46375 with CoRoT and ground-based support
    At the end of 2008, on ideas of teams from the Observatoire de la Côte d’Azur (OCA) and IAC, the CoRoT satellite observed the star HD 46375, known to host a non...
  • Charla
    Studying galaxies at low and high redshifts with GRBs
    Long gamma-ray bursts are supposed to be connected to the death of very massive stars. Due to their brightness, we can detect them to much larger distances than...
  • Charla
    Studying the Halo via Its NEarby low-mass Dwarfs
    Studying the Halo via Its NEarby low-mass Dwarfs (SHINED) is an ongoing project aiming to understand the Galactic halo with metal-deficient low-mass stars (LMS)...
  • Charla
    Studying the outer most regions of galaxies to constrain their formation
  • Charla
    Super Ifu Deployable Experiment: Project Status
    SIDE (Super Ifu Deployable Experiment) is being proposed as a new instrument for the GTC 10.4m telescope on La Palma. It will be a wide-field fiber-fed...
  • Charla
    Supergiant Stars as Extragalactic Probes of Cosmic Abundances and Distances
    The determination of chemical composition and distances of galaxies is crucial for constraining the theory of galaxy formation and evolution in a dark energy...