EPJ Web of Conferences
Volume 19, 2012Assembling the Puzzle of the Milky Way
|Number of page(s)||3|
|Section||Disc Assembly: Chemo-Dynamical Evolution, Radial Mixing|
|Published online||07 February 2012|
First results for the solar neighborhood of the Asiago Red Clump Survey
1 Institute d’Astrophysique et de Géophysique, Université de Liége, 4000 Liège, Belgium
2 INAF-OAPD-Osservatorio Astronomico di Padova, via dell’Osservatorio 8, 36012 Asiago, Italy
3 Mount Stromlo Observatory, Australian National University, Weston Creek, ACT 2611, Australia
4 University College London, Dept. of Space & Climate Physics, Mullard Space Science Lab., UK
5 Astronomisches Recheninstitut, Universitaet Heidelberg, Heidelberg, Germany
a e-mail: firstname.lastname@example.org
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.
© Owned by the authors, published by EDP Sciences, 2012
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