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Explore the critical role of stellar winds in binary-stripped star evolution through this 15-minute conference talk examining first wind mass loss measurements. Learn how gravitational wave detections, Gaia observations of dormant black holes, microlensing studies, and time domain surveys are revolutionizing our understanding of stellar mass black hole populations. Discover how these new observational data are compelling researchers to reassess the complete lifecycle of stellar black holes, from their massive star progenitors through core collapse and associated transients to their afterlives as dormant or accreting black holes and potential gravitational wave merger sources. Gain insights into cutting-edge research that bridges observational astronomy with theoretical stellar evolution models, presented as part of a comprehensive program bringing together experts to develop new observational and theoretical strategies for understanding stellar black hole lifecycles.
