A main sequence for quasars
Aula GrattonThe last 15 years have seen a major step forward in the analysis of optical
10 eventi found.
A main sequence for quasars
Aula GrattonThe last 15 years have seen a major step forward in the analysis of optical
The challenge of massive black hole binary coalescence; from galaxy formation to gravitational waves
Aula GrattonI will review recent progress in understanding how a pair of massive black holes can
The challenge of massive black hole binary coalescence; from galaxy formation to gravitational waves
Aula GrattonI will review recent progress in understanding how a pair of massive black holes can
AGB dust production: what we learn from the Local Group galaxies
Aula GrattonAsymptotic giant branch (AGB) stars are among the most important gas and dust polluters of
AGB dust production: what we learn from the Local Group galaxies
Aula GrattonAsymptotic giant branch (AGB) stars are among the most important gas and dust polluters of
From the first stars to the first quasars
Aula GrattonObservations of the most luminous quasars at redshift z>6 reveal the existence of numerous supermassive
From the first stars to the first quasars
Aula GrattonObservations of the most luminous quasars at redshift z>6 reveal the existence of numerous supermassive
Highly Ionized X-ray Absorbers in AGNs and their Energetic: the case of NGC 4051
Aula GrattonHighly ionized absorbers are found in 50% of type 1 Seyferts and QSOs. They presence,
Highly Ionized X-ray Absorbers in AGNs and their Energetic: the case of NGC 4051
Aula GrattonHighly ionized absorbers are found in 50% of type 1 Seyferts and QSOs. They presence,