Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S314(10), p. 205-206, 2015
DOI: 10.1017/s1743921315006286
Full text: Unavailable
AbstractUsing semi-empirical isochrones, we find the age of the Taurus star-forming region to be 3-4 Myr. Comparing the disc fraction in Taurus to young massive clusters suggests discs survive longer in this low density environment. We also present a method of photometrically de-reddening young stars using iZJH data.