Kinematic Distances of Pre-main Sequence Stars in the Lupus Star-Forming Region - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Revista Mexicana de Astronomia y Astrofisica Année : 2014

Kinematic Distances of Pre-main Sequence Stars in the Lupus Star-Forming Region

Résumé

IThe problem of the determination of distances has always played a central role in astronomy. However, little recent progress has been made in the distance determination of faint young stellar objects such as pre-main sequence (PMS) stars. Many of the PMS stars were neither observed by the Hipparcos satellite due to their magnitude nor have any trigonometric parallax measured from the ground due to their distance. Here we investigate the kinematic properties of the Lupus moving group with the primary objective of deriving individual parallaxes for each group member of this star-forming region.
Fichier non déposé

Dates et versions

hal-01062030 , version 1 (09-09-2014)

Identifiants

Citer

P. A. B. Galli, R. Teixeira, P. Benevides-Soares, C. Ducourant, Claude Bertout. Kinematic Distances of Pre-main Sequence Stars in the Lupus Star-Forming Region. 2014RMxAC.43..77G - Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 43, pp. 77-78 (2014), 2013, France. pp.77-78. ⟨hal-01062030⟩
96 Consultations
0 Téléchargements

Partager

Gmail Facebook X LinkedIn More