ARCS: the Asiago Red Clump Spectroscopic Survey

Details ARCS: the Asiago Red Clump Spectroscopic Survey ARCS: the Asiago Red Clump Spectroscopic Survey

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374..205v&link_type=abstract

From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer

Astronomy and Astrophysics

Astronomy

Scientific paper

The Asiago Red Clump Spectroscopic survey derives from high resolution optical spectra accurate multi-epoch radial velocities and atmospheric parameters (T_{eff}, log g, [M/H], V_{rot}sin i, [α/Fe], ξ) for a well selected sample of ˜500 equatorial Red Clump stars belonging to the solar neighborhood. These results coupled with astrometric and photometric external data are used in investigation of galactic structure and dynamics.

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