Determination of the Parameters of a Nonlinear Kinematic Galactic Rotation Model Based on the Proper Motions and Radial Velocities of Stars from the Gaia DR3 Catalogue

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Abstract

We have solved the Ogorodnikov–Milne stellar-kinematics equations in the Galactic rectangular coordinate system based on the total velocities for a special sample of stars with radial velocities from the final Gaia Data Release 3 catalogue. We have found the region of applicability of the linear model and the regions that it describes poorly. We have constructed a second-order model that takes into account the peculiarities of stellar kinematics more accurately and showed its applicability for stars at distances up to 5 kpc.

About the authors

A. S. Tsvetkov

St. Petersburg State University

Email: a.s.tsvetkov@inbox.ru
198504, St. Petersburg, Russia

F. A. Amosov

St. Petersburg State University

Author for correspondence.
Email: amosov.f@mail.ru
198504, St. Petersburg, Russia

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