• Starting date: 2015/06/29
  • End: 2015/07/04

    • LOCATION: Sexten Primary School - Via Panorama 6, Sexten

    DETAILS

    The field of cosmological hydrodynamical simulations that include a variety of physical processes (e.g. cooling, star formation, energy feedback from various sources, etc.) has seen important advancements in the last years, bringing to a number of important results: realistic simulated disk galaxies, realistic mix of galaxy morphological types, realistic description of multi-wavelength properties of galaxy clusters and of the IGM.
    The meeting aims tat bringing together experts working on simulations of cosmic structures – galaxies, clusters and large scale cosmic web – to discuss the state-of-the-art in the field, with particular emphasis on ub-resolution description of relevant astrophysical processes. This will be a small, dedicated workshop of 30-35 participants with half of the working time dedicated to informal discussion and work sessions and half to presentations.
    The workshop will focus on the following topics:
    – state of the art in simulations of galaxies and galaxy clusters:
    – discussion on the different sub-resolution description of star
      formation and feedback
    – the role of such schemes in predicting observable properties of intergalactic
      and circumgalactic medium

    RELATED FILES

    Scientific Programme with contributions

    FEE

    To be defined

    WORKSHOP CODE FOR PAYMENT

    ORGANIZERS

    Organizing commettee:
    Stefano Borgani
    Pierluigi Monaco
    Giuseppe Murante