Multiplicity at the Very Low Mass End of the H-R Diagram
We review the properties of multiplicity of very low mass stars and brown dwarfs in different environments and at different ages. We will compare the main results of surveys performed in the field, where the objects are relatively old (1-5 Gyrs) and isolated, in the Pleiades young (~120 Myr) open cluster, and in the young (~5 Myr) Upper Scorpius OB
Bouy, H. et al.
Fecha de publicación:
0
2008