http://arxiv.org/abs/1509.00170
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.
B. Stelzer, A. Frasca and J. Alcala
Wed, 2 Sep 15
76/87
Comments: 4 pages, to appear in Proceedings IAU Symposium No. 314, Young Stars & Planets Near the Sun, 2015
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