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

Details Spectroscopic Survey of Late-type Stars Possible Members of Young Moving Groups Spectroscopic Survey of Late-type Stars Possible Members of Young Moving Groups

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003csss...12..828m&link_type=abstract

The Future of Cool-Star Astrophysics: 12th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun (2001 July 30 - August

Astronomy and Astrophysics

Astrophysics

3

Late-Type Stars, Moving Groups, Chromospheres, Abundances, Kinematic, Open Clusters And Associations

Scientific paper

We summarize here our ongoing high resolution echelle spectroscopic survey of late-type stars, identified in our htmladdnormallink{previous studies}{http://www.ucm.es/info/Astrof/skg_sag.html} as possible members of htmladdnormallink{young moving groups}{http://www.ucm.es/info/Astrof/skg.html}. The spectroscopic observations were taken during five observing runs: July 1999 (2.2m-FOCES, CAHA, Almería), 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.

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