基于Gaia DR3星表中恒星固有运动和径向速度的非线性星系旋转模型参数的确定

IF 1.1 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astronomy Letters-A Journal of Astronomy and Space Astrophysics Pub Date : 2023-11-28 DOI:10.1134/S1063773723060051
A. S. Tsvetkov, F. A. Amosov
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引用次数: 0

摘要

我们已经在银河系直角坐标系中求解了Ogorodnikov-Milne恒星运动学方程,该方程基于Gaia数据发布3最终目录中具有径向速度的特殊恒星样本的总速度。我们发现了线性模型的适用范围和它描述得不好的范围。我们建立了一个二阶模型,该模型更准确地考虑了恒星运动学的特点,并显示了它对距离达5千公里的恒星的适用性。
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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

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.

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来源期刊
CiteScore
1.70
自引率
22.20%
发文量
0
审稿时长
6-12 weeks
期刊介绍: Astronomy Letters is an international peer reviewed journal that publishes the results of original research on all aspects of modern astronomy and astrophysics including high energy astrophysics, cosmology, space astronomy, theoretical astrophysics, radio astronomy, extragalactic astronomy, stellar astronomy, and investigation of the Solar system.
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