Recent advances in general relativistic magnetohydrodynamic modeling of jets offer unprecedented insights into the inner workings of accreting black holes that power the jets in active galactic nuclei (AGN) and other accretion systems. I will present the results of recent studies that determine spin-dependence of jet power and discuss the implications for the AGN radio loud/quiet dichotomy and recent observations of high jet power in a number of AGN.
|Original language||English (US)|
|Journal||Journal of Physics: Conference Series|
|State||Published - Jan 1 2012|
|Event||Astronomy at High Angular Resolution 2011: The Central Kiloparsec in Galactic Nuclei, AHAR 2011 - Bad Honnef, Germany|
Duration: Aug 29 2011 → Sep 2 2011
ASJC Scopus subject areas
- Physics and Astronomy(all)