Halfway to Binary Black Holes - A Census of O+BH Binaries in 30 Doradus
Kavli Institute for Theoretical Physics via YouTube
Overview
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Explore a comprehensive census of O-type star and black hole binary systems in the 30 Doradus star-forming region through this 15-minute conference talk. Examine how gravitational wave detections are transforming our understanding of stellar mass black hole populations, while Gaia observations reveal dormant black holes in detached binary systems with stellar companions. Learn about microlensing techniques that probe isolated black holes and time domain surveys searching for transients that mark black hole formation or stellar interactions. Discover how these diverse detection methods are unveiling new black hole populations that complement the accreting black holes traditionally studied through X-ray and radio observations. Understand the complete lifecycle of stellar black holes, from their massive star progenitors through core collapse and associated transients, to their existence as dormant or accreting objects, and their potential fate as gravitational wave sources during mergers. Gain insights into current observational findings and theoretical strategies being developed to address fundamental questions about stellar black hole evolution, presented as part of a broader conference bringing together experts to review recent discoveries in stellar black hole research.
Syllabus
Halfway to binary black holes: A census of O+BH binaries in 30 Doradus | Kunal Deshmukh (KU Leuven)
Taught by
Kavli Institute for Theoretical Physics