Formato de una charla: Seminario

  • Charla
    Properties and evolutionary state of massive stars across the HR diagram
    The advanced stages of high-mass stars are characterized by episodic mass loss shed during phases of instability. Key for assigning these stars a proper...
  • Charla
    Properties of the dwarf galaxy population in galaxy clusters
    Dwarf galaxies, being the most numerous and fragile galaxy population, provide unique clues on both the formation of baryonic systems and the role played by the...
  • Charla
    Proposed Operations and Renovation of the JKT by the Southeastern Association for Research In Astronomy
    The Southeastern Association for Research in Astronomy (SARA) is a consortium of 11 US universities that currently remotely operates a 0.9 m telescope at Kitt...
  • Charla
    PT theory, alternative gravity theories, and cosmological parameter estimation. Alternative gravity models (CLASS)​​​​​​​​​​
  • Charla
    PT theory, alternative gravity theories, and cosmological parameter estimation. EFT, PT (CLASS)
  • Charla
    PT theory, alternative gravity theories, and cosmological parameter estimation:​​​​​​​​​​​​​. Cosmological parameter estimation (CLASS, HiCLASS, Montepython, COSMOMC)
  • Charla
    PT theory, alternative gravity theories, and cosmological parameter estimation:​​​​​​​​​​​​​. SPT, RPT
  • Charla
    Pulsations in massive stars
    Massive stars shape and drive our Universe. Many issues such as their formation, their stability and the mass loss effects for example, are nowadays far for...
  • Charla
    Pyroclastic Blowout: Dust Survival in Isolated versus Clustered Supernovae
    Following the current debate on the fate of SN-condensed dust grains, I will present a set of three-dimensional hydrodynamical simulations of the interaction of...