From AGB stars to Planetary Nebulae: what the ISM, stellar rotation, and companions can do
Aula GrattonAsymptotic giant branch (AGB) stars lose their envelopes by means of heavy mass-loss rates. Besides
Stellar Populations in Local and high redshift Universe
Aula GrattonSynthetic stellar libraries are quite popular to constrain the stellar pop- ulations (age and metallicity
Colloquium – Marianna Torelli
Aula Grattoncolloquium – Giuseppe Tanzella-Nitti
Aula GrattonStar formation in the Local Group
Aula GrattonUsing Hubble Space Telescope (HST) observations, we have identified and characterised almost 50,000 pre-main sequence
colloquium – Guido De Marchi
Aula GrattonWhen the going get tough… or: observation and laboratory work for life searching in other worlds
Aula Gratton"...if we never search, the chance of success is zero". This was the conclusion in
Flipping a fair coin to decipher the large-scale environment of radio galaxies
Aula GrattonThe role played by the large-scale environment in the nuclear activity of radio galaxies is