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Salomé Dibi details four different studies of accretion and emission processes around the galactic centre Sgr A*, a supermassive black hole located in the centre of the Milky Way. Dibi studies Sgr A* because it is the closest supermassive black hole and therefore provides incomparable observational data with which to test theories and predictions.

Event details of Accretion and emission of closest supermassive black hole
Date 1 July 2014
Time 10:00 -11:00
Location Agnietenkapel

S. Dibi, Studying MHD and Radiative Processes in Sagittarius A*.


Prof. R.A.M.J. Wijers


Dr S.B. Markoff


Oudezijds Voorburgwal 229 - 231
1012 EZ Amsterdam


This event is open to the public.