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, (2) INAF-OAPD -, Osservatorio Astronomico di Padova, (3) Mnt Stromlo Observatory
TL;DR
This paper presents initial findings from the Asiago Red Clump Survey, analyzing Red Clump stars near the Sun to identify and characterize stellar moving groups in the Galactic disk.
Contribution
It provides the first results from ARCS, offering new data on Red Clump stars' parameters and insights into local stellar kinematics.
Findings
Detection of stellar moving groups in the Solar Neighborhood
Characterization of the kinematic properties of Red Clump stars
Preliminary mapping of Galactic disk structures
Abstract
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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