RACE-OC project: rotation and variability in the<i>ϵ</i>Chamaeleontis, Octans, and Argus stellar associations
S. MessinaINAF-Catania Astrophysical Observatory, via S. Sofia, 78, 95123 Catania, ItalyS. DesideraINAF-Padova Astronomical Observatory, Vicolo dell’Osservatorio 5, 35122 Padova, ItalyA. C. LanzafameINAF-Catania Astrophysical Observatory, via S. Sofia, 78, 95123 Catania, ItalyM. TurattoINAF-Catania Astrophysical Observatory, via S. Sofia, 78, 95123 Catania, ItalyE. F. GuinanDept. of Astronomy and Astrophysics, Villanova University, Villanova, 19085 PA, USA
2011en
ABI
Annotatsiya
Context. Rotational properties of late-type low-mass members of associations of known age provide a fundamental source of information on stellar internal structure and its evolution.
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