M. Valentini, U. Munari, T. Saguner, K. Freeman, S. Pasetto, J. Montalban, E. K. Grebel
The Asiago Red Clump Spectroscopic Survey (ARCS) is an ongoing survey that
provides atmospheric parameters, distances and space velocities of a well
selected sample of Red Clump stars distributed along the celestial equator. We
used the ARCS catalog for a preliminary investigation of the Galactic disk in
the Solar Neighborhood, in particular we focused on detection and
characterization of moving groups.
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http://arxiv.org/abs/1111.3769
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