D. Montes, Fernández-Figueroa M.J., De Castro E., Cornide M., Latorre A.
Departamento de Astrofísica, UCM
2001, ASP Conf. Ser., 223, CD-1477,
The 11th Cambridge Workshop on Cool Stars, Stellar Systems,
and the Sun ,
(Challenges for the New Millennium),
(October 4th - 8th, 1999, Puerto de la Cruz, Tenerife, Spain),
We present a kinematic study of a large sample of
chromospherically active binaries (CAB)
in order to determine their membership to representative
young disk stellar kinematic groups: the
Local Association (Pleiades moving group, 20 - 150 Myr),
Ursa Mayor group (Sirius supercluster, 300 Myr),
Hyades supercluster (800 Myr),
IC 2391 supercluster (35 Myr) and
Castor moving group (200 Myr).
Precise measurements of proper motions and parallaxes taken from
Hipparcos Catalogue and published radial velocity measurements
are used to calculate Galactic space motions (U, V, W)
in order to determine the membership of the selected stars to the different
stellar kinematic groups.
Chromospherically active binaries members of young stellar kinematic groups
R. García López, R. Rebolo, M.R. Zapatero Osorio (eds.),
PS_file (text)
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PS_file (figs)
Catalogue of Late-type Stars in Young Stellar Kinematic Groups
Publications about SKG by the Stellar Activity Group (UCM)
Actividad estelar
Stellar kinematic groups
David Montes, dmg@astrax.fis.ucm.es