|
|
|
|
|
|
|
We describe here our ongoing high-resolution spectroscopic survey
of single late-type stars identified in Paper I:
(Montes et al. 2001, MNRAS 328, 45)
as members of
young stellar kinematic groups
(SKG)
(Local Association (20 - 150 Myr),
Ursa Mayor group (300 Myr),
Hyades supercluster (600 Myr),
IC 2391 supercluster (35 Myr) and
Castor Moving Group (200 Myr))
or as other young disk stars.
Information about this spectroscopic study can be found in Montes et al. 2001, A&A 379, 976; Montes et al. 2002, 12th Cool SSS; Montes & López-Santiago, 2003, Kluwer Acad. Pub., p. 293 ; López-Santiago, et al., 2003, A&A, 411, 489; López-Santiago & Montes, 2004, Calar Alto Newsletter N.7; López-Santiago 2005, Ph.D. thesis, UCM; Lopéz-Santiago, et al. 2006, ApJ, 643, 1160; López-Santiago, et al. 2009, A&A, 499, 129 López-Santiago, Montes et al. 2010, A&A, 514, A97. The spectra and derived parameters database will be publicly released in these pages. |
|
|
Analysis of individual stars
Other publicaciones about SKG can be found
here.
Comments and suggestions to:
Stellar kinematic groups