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This book covers how Active Galactic Nuclei (AGN) are fueled by gas (or stars), how we can account for the wide variety of AGN observed, from Seyfert/Liners to quasars, and for the two types (AGN 1 and 2) either through dust obscuration, and geometrical orientation arguments, or through intrinsic activity difference, qualitative or quantitative.

Produktbeschreibung
This book covers how Active Galactic Nuclei (AGN) are fueled by gas (or stars), how we can account for the wide variety of AGN observed, from Seyfert/Liners to quasars, and for the two types (AGN 1 and 2) either through dust obscuration, and geometrical orientation arguments, or through intrinsic activity difference, qualitative or quantitative.
Autorenporträt
Francoise Combes is an astrophysicist at Paris Observatory, working on galaxy formation and evolution, on dark matter models and active galactic nuclei. She has been a Professor at College de France since 2014, and a member of the French Academy of Sciences since 2004. She has been an editor for Astronomy & Astrophysics since 2003. She has received the Gold Medal of CNRS in 2020, and the L'Oreal-Unesco International award for women in Science in 2021.