T Tauri Disk Lifetime in the Lupus Association
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Este ítem está publicado en
Young Stars & Planets Near the Sun, Proceedings of the International Astronomical Union, IAU Symposium, Volume 314, pp. 191-192- held 11 - 15 May 2015 / U.S.A, Atlanta, GA (Cambridge University Press), J.H. Kastner, B. Stelzer, S.A. Metchev, eds, 2016-05-11, Atlanta. 2015-11, vol. 10, n° S314
Resumen en inglés
In a recent study, we derived individual distances for a sample of pre-main sequence stars that define the comoving association of young stars in the Lupus star-forming region. Here, we use these new distances to investigate ...Leer más >
In a recent study, we derived individual distances for a sample of pre-main sequence stars that define the comoving association of young stars in the Lupus star-forming region. Here, we use these new distances to investigate the mass and age distributions of Lupus T Tauri stars and derive the average disk lifetime in the Lupus association based on an empirical disk model.< Leer menos
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