The age of Taurus - environmental effects on disc lifetimes
classification
🌌 astro-ph.SR
keywords
taurusdiscyoungclusterscomparingdatade-reddeningdensity
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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.
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