OMEG 2017, International Symposium on Origin of Matter and Evolution of Galaxies, Daejeon, Korea, JUNE 27-30, 2017

Session

Session 5 (Chair: N. Tominaga)

28 Jun 2017, 09:30

Hotel ICC, Daejeon, Korea

70. Massive stars evolution and nucleosynthesis

Raphael Hirschi (Keele U.)

28/06/2017, 09:30

Oral Presentation

71. Evolution of massive binary stars and its implications for the chemical evolution

Sung-Chul Yoon (Seoul national university)

28/06/2017, 09:55

Oral Presentation

A large fraction of massive stars are found to be in close binary systems. Binary interactions including exchanges of mass and angular momentum via mass transfer and tidal synchronization can greatly affect the evolution of massive stars. This has many important implications for hydrogen-deficient supernovae, hypernovae, formation of compact binaries (neutron stars and black holes), and...