Marco Gatti: Triggering AGN activity in galaxies: galaxy interactions vs. disk instabilities
→
Europe/Madrid
Seminar (IFAE)
Seminar
IFAE
, ,
Description
In the last decades it has become widely accepted that Active Galactic Nuclei (AGN) are powered by the accretion of matter onto SuperMassive Black Holes (SMBHs), and that their evolution is tightly correlated with that of their host galaxies. However, the physical mechanisms responsible for such intense accretion episodes in the galactic nuclei still remain unclear.
A statistical study about the role of different triggering mechanisms can be performed using simulations such as semi-analytic models of galaxy formation. Two different main fueling mechanisms will be considered: a first mode where AGN activity is triggered by disk instabilities in isolated galaxies, and a second mode where the inflow onto the central SMBH is induced by galaxy interactions (i.e., galaxy mergers and fly-by events).
Participants
Alejandro Belloti
Bruno Bourguille
Chihaya Anzai
Daniel Moreno
Daniele Ninci
David Vázquez Furelos
de la Rosa Gloria
Emanuele Cavallaro
Enrique Fernandez
Fabian foerster
Federico Sanchez
Giuliano Panico
Hornung Dirk
Imma Riu
Jelena Aleksic
Joern Lange
John E Ward
Judit Prat
Ke Yang
Kovacs Andras
Leyre Nogués
Manel Martinez
Martine Bosman
Mateo Garcia
Matthias Jamin
Oscar Blanch Bigas
Oscar Martinez
Paolo Cumani
Quiros Mariano
Raimon Casanova
Ramon Miquel
Sergi Gonzalez-solis
Sergio Sanchez Cruz
Stefania Bordoni
Thibaud Vantalon
Thorsten Lux
Xabier Lobregat