J. M. Rees
The Age of Taurus: Environmental Effects on Disc Lifetimes
Rees, J. M.; Wilson, T.; Bell, C. P. M.; Jeffries, R. D.; Naylor, T.
Abstract
Using 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.
Citation
Rees, J. M., Wilson, T., Bell, C. P. M., Jeffries, R. D., & Naylor, T. (2015). The Age of Taurus: Environmental Effects on Disc Lifetimes. Proceedings of the International Astronomical Union, 10(S314), 205-206. https://doi.org/10.1017/s1743921315006286
Journal Article Type | Conference Paper |
---|---|
Online Publication Date | Jan 27, 2016 |
Publication Date | 2015-11 |
Deposit Date | Jun 16, 2023 |
Journal | Proceedings of the International Astronomical Union |
Print ISSN | 1743-9213 |
Electronic ISSN | 1743-9221 |
Publisher | Cambridge University Press |
Peer Reviewed | Peer Reviewed |
Volume | 10 |
Issue | S314 |
Pages | 205-206 |
DOI | https://doi.org/10.1017/s1743921315006286 |
Keywords | Astronomy and Astrophysics; Space and Planetary Science; stars: evolution, stars: pre-main sequence, stars: fundamental parameters |
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