GALLI, P. A. B.; TEIXEIRA, R.; DUCOURANT, C.; BERTOUT, C.

doi:10.1017/S1743921312021783

Métadonnées

Afficher la notice complète

Licence d’utilisation du document

GALLI, P. A. B.

TEIXEIRA, R.
Instituto de Astronomia, Geofísica e Ciências Atmosféricas [São Paulo] [IAG]

DUCOURANT, C.
M2A 2013

Langue

Communication dans un congrès

Ce document a été publié dans

Proceedings of the International Astronomical Union, Advancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013, Advancing the Physics of Cosmic Distances, Proceedings of the International Astronomical Union, IAU Symposium, Volume 289, pp. 390-393, 2013, Advancing the Physics of Cosmic Distances, 2012, beijing. 2013-02, vol. 289, p. 390-393

Cambridge University Press (CUP)

Résumé en anglais

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.< Réduire

Mots clés en anglais

stars: distances

stars: kinematics

stars: pre-main-sequence

ISM: individual (Lupus star-forming region)

Métadonnées

Licence d’utilisation du document

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

Langue

Ce document a été publié dans

Résumé en anglais

Mots clés en anglais

DOI

Origine

Unités de recherche