Prof.
Tomasz
Bulik
Astronomical Observatory, University of Warsaw
LVK has already detected nearly hundred of mergers not counting thecurrent O4 run. This allows us to investigate the properties of the detectedpopulation. I will review what we know of the detections, present thepossible models of formation of these objects, and compare the modelswith observations.
This is a hybrid event:
Room D, the Institute of Physics PAS, Al. Lotników 32/46
Online: Zoom Link, (Passcode: 134595, Meeting ID: 823 8038 0442)
