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SUMMARY:The effect of binary mass transfer on the late evolution\, death\,
  and afterlife of massive stars - Eva laplace\, University of Leuven\, Bel
 gium
DTSTART:20250522T150000Z
DTEND:20250522T160000Z
UID:TALK232012@talks.cam.ac.uk
CONTACT:130201
DESCRIPTION:Gravitational-wave observations have revealed the population o
 f stellar remnants from a new angle. Yet their stellar progenitors remain 
 uncertain\, in particular in the case of black holes. At least a fraction 
 of these stars is believed to form in isolated binary systems. In this tal
 k\, I will discuss how binary mass transfer affects the late evolution and
  final fate of massive stars. The focus will be on stars that transfer the
 ir outer layers to a companion star and become binary-stripped. Binary-str
 ipped stars develop systematically different core structures compared to s
 ingle stars. I will discuss consequences for supernovae\, black hole forma
 tion\, and gravitational-wave observations.
LOCATION:Hoyle Lecture Theatre\, Institute of Astronomy
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