Year: 2024
Type: article
Abstract: The kinematic properties of the Sco-Cen association are studied using the spatial velocities of young stars. New kinematic age estimates for the three components of the association were obtained, with the age of UCL and LCC being 17.7 ± 2.4 Myr, and the age of US being 6.4 ± 1.7 Myr. The parameters of the residual velocities US, UCL and LCC were estimated.
Source: Astronomicheskii Zhurnal
Authors: V. V. Bobylev, A. T. Bajkova
Institutions: Russian Academy of Sciences, Pulkovo Observatory
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W4406073696