Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S314(10), p. 105-108, 2015
DOI: 10.1017/s174392131500633x
Full text: Unavailable
AbstractWe present new photometric and spectroscopic data for the M-type members of the TW Hya association with the aim of a comprehensive study of accretion, disks and magnetic activity at the critical age of ~ 10 Myr where circumstellar matter disappears.