  A limited-area survey of the eta Chamaeleontis cluster has identified 2 new
late-type members. The more significant of these is ECHA J0843.3-7905 (= IRAS
F08450-7854), a slowly-rotating (P = 12 d) M2 classical T Tauri (CTT) star with
a spectrum dominated by Balmer emission. At a distance of 97 pc and cluster age
of approx 9 Myr, the star is a nearby rare example of an 'old' CTT star and
promises to be a rewarding laboratory for the study of disk structure and
evolution in pre-main sequence (PMS) stars. The other new member is the M4
weak-lined T Tauri (WTT) star ECHA J0841.5-7853, which is the lowest mass (M =
0.2 M_sun) primary known in the cluster.
