| Chromospherically active binaries members of young open clusters |
D. Montes
Departamento de Astrofísica, UCM
2000, ASP Conf. Ser. 198, 475, in
"Stellar clusters and associations: convection, rotation, and dynamos",
(Second "Three-Islands" Euroconference) (May 25 - 28, 1999, Mondello, Palermo, Sicily, Italy),
R. Pallavicini, G. Micela and S. Sciortino eds.
PS_file
We have compiled a list of
late-type stars (F5-M) spectroscopic binaries members of nearby
and well-studied young open clusters:
Persei (51 Myr),
Pleiades (77 Myr), Coma Berenices (500 Myr),
Hyades (660 Myr), Praesepe (660 Myr).
Stars have been selected making use of the information provided by
open clusters databases and
the most recent literature.
Many of these systems are chromospherically active binaries (CAB),
other are possible CAB,
but their activity indicators need to be confirmed.
Basic stellar parameters and references for orbital parameters
are listed for each star.
Preliminary lists of late-type spectroscopic binaries members of young open clusters can be found here:
Actividad estelar
Open clusters