Talk format: Seminar

  • Talk
    The rich population of jellyfish galaxies in Abell 901/2 at z ~ 0.165
    The bimodal distribution of red and blue galaxies can often be linked through a quenching mechanism that can attenuate the active star forming galaxies into...
  • Talk
    The role of black holes in regulating star formation
    Black holes are a fundamental ingredient in our current understanding of galaxy formation. In the absence of their feedback, state-of-the-art numerical...
  • Talk
    The role of massive black hole recoil in galaxy evolution
    The coalescence of a massive black hole (MBH) binary leads to the gravitational-wave recoil of the system and its ejection from the galaxy core. We have carried...
  • Talk
    The Rugged Landscape of Core-Collapse Supernova Explosions
    The collapse of the core and the associated supernova explosion mark the end of life of most massive stars, but the mechanism of explosion is poorly understood...
  • Talk
    The SARA Consortium: A Virtual Astronomy Department
    For over 20 years, the Southeastern Association for Research in Astronomy (SARA) has operated a remotely-accessible 1-m-class telescope at the Kitt Peak...
  • Talk
    The Scaling Relations of Cluster Galaxies
    Major tests of cosmological and galaxy formation models can be constructed through dynamical and structural parameters of galaxies. Towards this end, we present...
  • Talk
    The Scutum-Crux Complex: Tying massive stellar formation with the overall structure of the Milky Way
    With the discovery of several massive, young clusters in the last five years, the area around the base of the Scutum-Crux arm (around l=28) has become one of...
  • Talk
    The search for habitable Earth-like planets
    The search of Earth-like extrasolar planets approaches a key moment in its history. With the arrival of ESPRESSO (observing already!), the possibility of...
  • Talk
    The Sigma Orionis cluster: from 20 Msun to free-floating planets
    For the first time, we present the low-mass function of the entire young star cluster Sigma Orionis (3 Myr, 352 pc, no internal extinction) from 0.25 Msun...