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• W3100926031 abstract "We present the results of an age determination study of pre-main sequence stars in the Taurus star-forming region. The ages of 10 single stars with masses of 0.5-1.1 Msun were derived from the surface gravities, estimated from high-resolution optical and near-infrared spectroscopy. The equivalent width ratios of nearby absorption line pairs were employed for the surface gravity diagnostic, which directly reflects the parameters of the stellar atmosphere without any veiling correction. From a comparison of determined ages and near-infrared color excesses such as J-H, J-K, and J-L, the inner disk lifetime of the young stars with 0.5-1.1 Msun in Taurus is estimated to be 3-4 Myr." @default.
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• W3100926031 date "2014-09-17" @default.
• W3100926031 modified "2023-09-26" @default.
• W3100926031 title "Disk dissipation timescale of pre-main sequence stars in Taurus*" @default.
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• W3100926031 doi "https://doi.org/10.1093/pasj/psu062" @default.
• W3100926031 hasPublicationYear "2014" @default.
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