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“…Most methods used today require stellar evolutionary models one way or another and still have large uncertainties. With advances in stellar modelling and precise distances (e.g., Perryman et al 1997), it is only relatively recently that deriving ages for large number of field stars has become possible. The most common way of deriving stellar ages is by isochrone fitting (e.g., Jørgensen & Lindegren 2005;Yi et al 2001).…”
Section: Introductionmentioning
confidence: 99%
“…Most methods used today require stellar evolutionary models one way or another and still have large uncertainties. With advances in stellar modelling and precise distances (e.g., Perryman et al 1997), it is only relatively recently that deriving ages for large number of field stars has become possible. The most common way of deriving stellar ages is by isochrone fitting (e.g., Jørgensen & Lindegren 2005;Yi et al 2001).…”
Section: Introductionmentioning
confidence: 99%