Kinematics of the Milky Way from the Statistical Analysis of the Gaia Data Release 3

The aim of the analysis of data from the Gaia Space Observatory is to obtain kinematic parameters of the collective motion of stars in a part of our galaxy. This research is based on a statistical analysis of the motion of <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML...

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Bibliographic Details
Main Authors: Petr Zavada, Karel Píška
Format: Article
Language:English
Published: MDPI AG 2025-02-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/13/1/10
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