Kinematics of Fainst Stars of the Sco-Cen Association According to Gaia Catalog
Vadim V. Bobylev, Anisa T. Bajkova
TL;DR
This study analyzes the kinematic properties of the Sco-Cen association's young stars using Gaia data, providing new age estimates and residual velocity parameters for its components.
Contribution
It offers novel kinematic age estimates and residual velocity parameters for the Sco-Cen association's components based on Gaia data.
Findings
UCL and LCC ages estimated at 17.7±2.4 Myrs
US age estimated at 6.4±1.7 Myrs
Parameters of residual velocities for US, UCL, and LCC ellipsoids
Abstract
The kinematic properties of the Sco-Cen association have been studied using the spatial velocities of young stars. New kinematic age estimates for the three components of the association with the age of UCL and LCC being Myrs and the age of US being Myrs have been obtained. The parameters of the residual velocities US, UCL, and LCC ellipsoid have been estimated.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.