POSTER PAPER 4.16

Spectroscopic Survey of Late-type Stars Possible Members of Young Moving Groups
D. Montes, J. Lopez-Santiago, M.C. Galvez, M.J. Fernandez-Figueroa, M. Cornide, E. De Castro

Institute: Dpto Astrofisica, Universidad Complutense de Madrid
Contact Email: dmg@astrax.fis.ucm.es

Abstract: We summarize here our ongoing high resolution echelle spectroscopic survey of late-type stars, identified in our previous studies as possible members of young moving groups. The spectroscopic observations were taken during five observing runs: July 1999 (2.2m-FOCES, CAHA, Almeria), November 1999 and 2000 (NOT-SOFIN, La Palma), and January 2000 and August 2000 (INT-MUSICOS , La Palma). Our main goal is to analyse in more detail the membership of these stars to the different young stellar kinematic groups.

Spectroscopic Survey of Late-type Stars Possible Members of Young Moving Groups [PDF - Type 1 fonts]

Spectroscopic Survey of Late-type Stars Possible Members of Young Moving Groups [PS]


Index Keywords: Late-type Stars; Moving Groups; Chromospheres; Abundances; Kinematic; Open Clusters and Associations

Previous: Glebocki Next: De Medeiros
Up: Poster Index Up: Top Index


Manuscript submitted: 2001-Sep-06
"The Future of Cool-Star Astrophysics", 2003, Eds. A. Brown, G. M. Harper, & T. R. Ayres. Proceedings of 12th Cambridge Workshop on Cool Stars, Stellar Systems, & The Sun,
© 2003 University of Colorado.