Volume 552, April 2013
|Number of page(s)||8|
|Section||Stellar structure and evolution|
|Published online||19 March 2013|
1 Instituto de Astrofísica de Canarias (IAC), 38205 La Laguna, Tenerife, Spain
2 Departamento de Astronomía, Universidad de Chile, Casilla Postal 36D, Santiago, Chile
3 Center for Astrophysics Research, University of Hertfordshire, College Lane, Hatfield, Herts, AL10 9AB, UK
Received: 25 April 2012
Accepted: 13 February 2013
We present the results of a study of the stellar activity in the solar neighborhood using complete kinematics (galactocentric velocities U, V, W) and the chromospheric activity index log R'HK. We analyzed the average activity level near the centers of known moving groups using a sample of 2529 stars and found that the stars near these associations tend to be more active than field stars. This supports the hypothesis that these structures, or at least a significant part of them, are composed of kinematically bound, young stars. We confirmed our results by using GALaxy Evolution EXplorer (GALEX) UV data and kinematics taken from the Geneva-Copenhagen Survey for the stars in the sample. Finally, we present a compiled catalog with kinematics and activities for 2529 stars and a list of potential moving group members selected based on their stellar activity level.
Key words: stars: activity / stars: kinematics and dynamics / stars: solar-type / solar neighborhood
Table 4 is available in electronic form at http://www.aanda.org
Full Table 1 is only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (188.8.131.52) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/552/A27
© ESO, 2013
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