How to tackle a giant Star: multi-wavelength studies of cool, evolved stars, using HST and VLTI
Aula GrattonThe chemical enrichment of the Universe is considerably affected by the contributions of Giant stars.
An infrared and sub-mm view of AGN obscuration and feedback
Aula GrattonIn the past 10-15 years our view of AGN has significantly evolved thanks to the
colloqium – Cristina Ramos Almeida
Aula GrattonClustering dependence of X-ray AGN on host galaxy properties
Aula GrattonThe presence of a super massive BH in almost all galaxies in the Universe is
colloquium – Viola Allevato
Aula GrattonMultimessenger astrophysics with active galactic nuclei: observational clues of gamma-neutrino connection in blazars
Aula GrattonThe clear detection of an isotropic flux of very high energy neutrinos by the IceCube
colloquium – Antonio Stamerra
Aula GrattonUltraviolet imager with wide-field & deep for astronomical observation and study
Aula GrattonBase on the ultraviolet radiation characteristics of cosmic celestial models and different morphological materials, the
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