Multiplicity among the cool supergiants in the Magellanic Clouds
The characterization of multiplicity of high-mass stars is of fundamental importance to understand their evolution, the diversity of observed core-collapse supernovae and the formation of gravitational wave progenitor systems. Despite that, until recently, one of the final phases of massive star evolution - the cool supergiant phase - has received
Dorda, R. et al.
Fecha de publicación:
4
2021