The IACOB project: searching for empirical signatures of binarity in fast-rotating Galactic O stars and B supergiants
Rotation is one of the important parameters affecting the evolution and final fate of massive stars. Still the origin of fast- rotating stars in the massive OB domain remains unclear. Although the high spin rates detected in about 20-30% of these stars could just be an imprint of the star formation process, alternative scenarios -supported by the
Britavskiy, N. et al.
Fecha de publicación:
7
2020