[en] 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.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Valentini, Marica ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Munari, U.; INAF-OAPD-Osservatorio Astronomico di Padova, via dell'Osservatorio 8, 36012, Asiago, Italy
Saguner, T.; INAF-OAPD-Osservatorio Astronomico di Padova, via dell'Osservatorio 8, 36012, Asiago, Italy
Freeman, K.; Mount Stromlo Observatory, Australian National University, Weston Creek, ACT 2611, Australia
Pasetto, S.; University College London, Dept. of Space & Climate Physics, Mullard Space Science Lab., UK ; Astronomisches Recheninstitut, Universitaet Heidelberg, Heidelberg, Germany
Montalban Iglesias, Josefa ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique et astérosismologie
Grebel, E. K.; Astronomisches Recheninstitut, Universitaet Heidelberg, Heidelberg, Germany)
Language :
English
Title :
First results for the solar neighborhood of the Asiago Red Clump Survey
