|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
Weighing Supermassive Black Holes from Zero to High Redshift
If you have a question about this talk, please contact David Titterington.
*** Note change of time
Supermassive black holes are believed to grow during bright AGN phases and are considered key players in the formation and evolution of galaxies. Black hole masses are thus fundamental physical quantities to characterise AGN activity and host galaxies. In this talk I will briefly review the accuracy and reliability of black holes mass measurements from zero to high redshift and present new results on virial estimators, currently the only way to measure black hole masses beyond the local universe. I will then discuss the redshift evolution of the scaling relations between BHs and their host galaxies, as derived from the application of these virial estimators, and the constraints we can infer for galaxy evolutionary models.
This talk is part of the Cavendish Astrophysics Seminars series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsBritish Epigraphy Society Cambridge Statistics Initiative (CSI) Mind-matter Unification Project (TCM Group, Cavendish Laboratory)
Other talksMerck, Sharp & Dohme Lecture Antihypertensive medication in normotensive elderly patients: a way forward in the prevention of dementia? Oxidative stress, ROS and free radicals - using nitroxide antioxidants for detection and protection Hydrogen–deuterium exchange mass spectrometry Can neurocognitive findings inform our understanding of disruptive behavior and what to do with it? Thelocactus