First Results for the Solar Neighborhood of the Asiago Red Clump Survey

(2) INAF-OAPD - Osservatorio Astronomico di Padova; (3) Mnt Stromlo Observatory; (4) University College London - Dept. of Space; 5); (5) Astronomisches Recheninstitut; Australian National University; Climate Physics; E. K. Grebel (5) ((1) Institute d'Astrophysique et de Geophysique - Universite' de Liege; J. Montalban (1); K. Freeman (3)

arxiv: 1111.3769 · v1 · pith:NPTTX4V6new · submitted 2011-11-16 · 🌌 astro-ph.GA

First Results for the Solar Neighborhood of the Asiago Red Clump Survey

M. Valentini (1) , U. Munari (2) , T. Saguner (2) , K. Freeman (3) , S. Pasetto (4 , 5) , J. Montalban (1) , E. K. Grebel (5) ((1) Institute d'Astrophysique et de Geophysique - Universite' de Liege

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(2) INAF-OAPD - Osservatorio Astronomico di Padova (3) Mnt Stromlo Observatory Australian National University (4) University College London - Dept. of Space Climate Physics (5) Astronomisches Recheninstitut Universitaet Heidelberg)

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keywords clumpsurveyarcsasiagoneighborhoodsolaralongatmospheric

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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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First Results for the Solar Neighborhood of the Asiago Red Clump Survey

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