CORDIS Project
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This project investigates common envelope evolution in massive binary systems by studying luminous red novae as indicators of this process. It aims to enhance our understanding of the physical mechanisms involved in binary evolution and their implications for astrophysics using advanced observational techniques.
Common envelope evolution (CEE) is a crucial phase in binary evolution, as it is responsible for the formation of many of the most exciting systems in astrophysics, including sources of gravitational waves.
Despite its importance, there are several unanswered questions that hamper the urgently needed progress in this field:
What systems enter CEE?
What happens during CEE?
How the CEE remnants evolve?
Recently, a new type of astrophysical transients called luminous red novae (LRNe) has emerged as…
UNIVERSITAT DE BARCELONA
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