LkHα 262/263: the paradigm of multiplicity vs disk fraction in low-mass stellar systems.
The study of multiple systems and their link with the presence of discs around their components is key to understanding the evolution of low-mass pre-main sequence stars. Although there are indications that high-multiplicity systems are much more frequent among very young stars, until now, only a few of these young low-mass stellar systems have
Velasco, S. et al.
Fecha de publicación:
3
2017