Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S314(10), p. 205-206, 2015

DOI: 10.1017/s1743921315006286

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The Age of Taurus: Environmental Effects on Disc Lifetimes

Journal article published in 2015 by J. M. Rees, T. Wilson ORCID, C. P. M. Bell, R. D. Jeffries, T. Naylor ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Abstract

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.

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