Accretion, disks, and magnetic activity in the TW Hya association
arXiv:1509.00170 · doi:10.1017/S174392131500633X
Abstract
We 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.
4 pages, to appear in Proceedings IAU Symposium No. 314, Young Stars & Planets Near the Sun, 2015