Kinematic distances of pre-main-sequence stars in the Lupus star-forming region

P. A. B. Galli R. Teixeira 1 C. Ducourant 2 C. Bertout
2 M2A 2013
L3AB - Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux, OASU - Observatoire aquitain des sciences de l'univers, LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac], Université Sciences et Technologies - Bordeaux 1
Abstract : To reliably determine the main physical parameters (masses and ages) of young stars, we must know their distances. While the average distance to nearby star-forming regions (<300 pc) is often known, the distances to individual stars are usually unknown. Individual distances to members of young moving groups can be derived from their radial velocities and proper motions using the convergent-point strategy. We investigate the kinematic properties of the Lupus moving group with the primary objective of deriving individual distances to all group members.
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Contributeur : Marie-Paule Pomies <>
Soumis le : lundi 10 juin 2013 - 14:48:03
Dernière modification le : lundi 26 novembre 2018 - 17:20:02

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P. A. B. Galli, R. Teixeira, C. Ducourant, C. Bertout. Kinematic distances of pre-main-sequence stars in the Lupus star-forming region. Advancing the Physics of Cosmic Distances, 2012, beijing, China. 289, pp.390-393, 2013, 〈10.1017/S1743921312021783〉. 〈hal-00832298〉



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