Formato de una charla: Seminario

  • Charla
    CMB cross-correlations with LSS. Component separation methods and forecasting of r-detectability with future experiments
  • Charla
    CMB cross-correlations with LSS. Introduction to CMB, CMB clusters
  • Charla
    CMB cross-correlations with LSS. kSZ, ISW
  • Charla
    CMB cross-correlations with LSS. Polarized foregrounds
  • Charla
    CMB cross-correlations with LSS. Spectral distortions
  • Charla
    CMB cross-correlations with LSS. Theory of CMB polarization, and current status of CMB polarization measurements
  • Charla
    Cold flow accretion into galaxies
    The flow of gas from the cosmic web into galaxies provides the necessary fuel for star formation and galaxy assembly. I will review our current knowledge about...
  • Charla
    Cold streams: detectability, relation to structure and characteristics
    Cold gas streaming along the dark-matter filaments of the cosmic web is predicted to be the major provider of resources for disc buildup and star formation in...
  • Charla
    Collisional phenomena in the lower solar atmosphere
    The lower solar atmosphere is very weakly ionized, and by conductivity it is comparable to the sea water. The collisional frequency for electrons and ions can...