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Sara Elisa Motta (Istituto Nazionale di Astrofisica (INAF))16/06/2026, 12:15Talk
The inflow of matter onto astronomical objects is connected to the generation of outflows throughout the Universe on a variety of scales, from proto-planetary disks, to merging neutron star systems and gamma ray bursts, to stellar mass and supermassive black holes.
The matter inflow/outflow processes scale predictably with mass, and proceeds according to the same basic principles around all...
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Elisa Bortolas16/06/2026, 14:35Talk
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Dr Ilaria Ruffa (INAF - OAA)16/06/2026, 14:55Talk
The last three decades of observations have demonstrated that the mass of central super-massive black holes (SMBHs) correlates with a number of properties of their host galaxies, suggesting a connection between the growth of these massive compact objects and their host galaxy evolution (so-called "co-evolution”). Galaxy formation theories, however, still struggle to shed light on the physical...
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Dr Gabriele Bruni (INAF - Istituto di Astrofisica e Planetologia Spaziali)16/06/2026, 15:10Talk
Recent time-domain surveys are revealing a growing population of nuclear transients that trace rapid changes in the accretion state of supermassive black holes. These events offer a unique opportunity to study how previously quiescent or weakly active nuclei transition into phases of enhanced accretion and variability. In this contribution I will present recent multiwavelength results on a...
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Francesca Onori (Istituto Nazionale di Astrofisica (INAF))16/06/2026, 15:25Talk
When an unfortunate star wanders too close to a Super Massive Black Hole (SMBH) it can be destroyed by the strong tidal forces at play. These Tidal Disruption Events (TDE) are powerful transient sources which reveal the presence of dormant SMBHs in the low-mass regime. Thus, they represent an extraordinary laboratory for studying the properties of a population of SMBHs complementary to the...
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Ms Maya Garbaccio Gili (Istituto Nazionale di Astrofisica (INAF))16/06/2026, 15:40Talk
Intermediate-mass black holes (IMBHs) constitute the missing link between stellar-mass and supermassive black holes (BHs). As such, they are crucial to trace BH growth and its connection with galaxy evolution. However, their presence in the local universe remains elusive: less than a dozen X-ray-bright IMBH candidates have been found so far. Among these, ESO243-49 HLX-1 stands out as one of...
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Maurizio Paolillo (Università di Napoli Federico II)16/06/2026, 15:55Talk
The combination of past and new monitoring optical surveys is allowing to probe the intrinsic properties of accreting supermassive black holes through variability studies. I will present results of the Timedomes campaign to target the LSST Deep Drilling Fields in order to assemble a legacy dataset of AGN lightcurves going back more than 10 years down to magnitude limits comparable with LSST...
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