Kinematics of the Local Stellar System

Research output

Abstract

The paper presents an overview of the results derived from application of the Ogorodnokov-Shatsova model of the Local Stellar system (LSS) rotation to the data of the HIPPARCOS catalogue. The most probable values of the geometric parameters are found. It is proved that the pole of the LSS rotation deviates from the Galactic pole by 20-30 degrees. The most probable values of the rotation parameters are found. It is shown that the LSS rotates in the opposite directions with respect to the Galaxy rotation. The outer border of the LSS have been traced up to 200-300 pc. For more distant stars the Galactic rotation dominates in the proper motions. It was found that the LSS consists not only of the OB-stars but includes the A-F stars as well. The K-M stars (nor giants neither dwarfs) are the members of the LSS.
Original languageEnglish
Title of host publicationProc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg.
Publication statusPublished - 2000

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stellar systems
kinematics
poles
F stars
galactic rotation
K stars
A stars
stars
M stars
proper motion
borders
catalogs
galaxies

Cite this

Tsvetkov, A. S. (2000). Kinematics of the Local Stellar System. In Proc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg.
Tsvetkov, A.S. / Kinematics of the Local Stellar System. Proc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg.. 2000.
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Tsvetkov, AS 2000, Kinematics of the Local Stellar System. in Proc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg..

Kinematics of the Local Stellar System. / Tsvetkov, A.S.

Proc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg.. 2000.

Research output

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T1 - Kinematics of the Local Stellar System

AU - Tsvetkov, A.S.

PY - 2000

Y1 - 2000

N2 - The paper presents an overview of the results derived from application of the Ogorodnokov-Shatsova model of the Local Stellar system (LSS) rotation to the data of the HIPPARCOS catalogue. The most probable values of the geometric parameters are found. It is proved that the pole of the LSS rotation deviates from the Galactic pole by 20-30 degrees. The most probable values of the rotation parameters are found. It is shown that the LSS rotates in the opposite directions with respect to the Galaxy rotation. The outer border of the LSS have been traced up to 200-300 pc. For more distant stars the Galactic rotation dominates in the proper motions. It was found that the LSS consists not only of the OB-stars but includes the A-F stars as well. The K-M stars (nor giants neither dwarfs) are the members of the LSS.

AB - The paper presents an overview of the results derived from application of the Ogorodnokov-Shatsova model of the Local Stellar system (LSS) rotation to the data of the HIPPARCOS catalogue. The most probable values of the geometric parameters are found. It is proved that the pole of the LSS rotation deviates from the Galactic pole by 20-30 degrees. The most probable values of the rotation parameters are found. It is shown that the LSS rotates in the opposite directions with respect to the Galaxy rotation. The outer border of the LSS have been traced up to 200-300 pc. For more distant stars the Galactic rotation dominates in the proper motions. It was found that the LSS consists not only of the OB-stars but includes the A-F stars as well. The K-M stars (nor giants neither dwarfs) are the members of the LSS.

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KW - Galaxy rotation

KW - Hipparcos

M3 - Article in an anthology

BT - Proc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg.

ER -

Tsvetkov AS. Kinematics of the Local Stellar System. In Proc. of the Conference "Stellar dynamics: from classic to modern", August 2000, St.Petersburg.. 2000