Splinter Meeting AGN
Active Galactic Nuclei
Time: Wednesday September 20, 14:00-16:30
Organizers: Wolfram Kollatschny (Göttingen), Martin Haas (Bochum), Helmut Meusinger (TLS Tautenburg), Michael Ramolla (Bochum), Matthias Zetzl (Göttingen)
Active Galactic Nuclei (AGN) are understood as supermassive black holes (SMBH) that accrete large amounts of matter to sustain their immense variable luminosity seen at all frequency ranges. This splinter meeting will address open questions regarding the structure and evolution of AGN as well as their interaction with the environment.
Related contributions *)
|Britzen||OJ287 - Deciphering the Rosetta stone of blazars||Talk|
|Ghaffari||Galaxy overdensities around 3C radio galaxies and quasars at 1||Talk|
|Marian||Testing the connection between major mergers and the triggering of high-accretion black holes||Talk|
|Nunez||Optical Photometric Monitoring of Active Galactic Nuclei at Wise Observatory||Talk|
|Puchwein||The role of AGN in cosmic reionization||Talk|
|Schindler||The Extremely Luminous Quasars Survey (ELQS) in SDSS||Talk|
|Sobrino-Figaredo||IC4329A: a red Seyfert-1 nucleus in an edge-on host galaxy||Talk|
|Vardoulaki||FR-type radio sources in COSMOS: relation to size, accretion modes and large-scale environment||Talk|
|Zetzl||Line profile variations in the changing look AGN HE 1136-2304||Talk|
*) submitted abstracts, acceptance pending.