ISM Lecture 10 The Three-Phase Interstellar Medium 10.1 Why necessary? Two-phase model (see Sect. 8.3) FGH model: Heating by cosmic rays => p.e. effect UV from stars:…
Panchromatic population synthesis studies of galaxies Laura Silva –INAF Trieste Alessandro Bressan – INAF Padova Gian Luigi Granato – INAF Padova Pasquale Panuzzo –INAF…