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

Proceedings of the IV international workshop on positional astronomy and celestial mechanics. Universitat de Valencia, 1998. p. 73-80.

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Harvard

Tsvetkov, AS 1998, Kinematics of the Local Stellar system. in Proceedings of the IV international workshop on positional astronomy and celestial mechanics. Universitat de Valencia, pp. 73-80.

APA

Tsvetkov, A. S. (1998). Kinematics of the Local Stellar system. In Proceedings of the IV international workshop on positional astronomy and celestial mechanics (pp. 73-80). Universitat de Valencia.

Vancouver

Tsvetkov AS. Kinematics of the Local Stellar system. In Proceedings of the IV international workshop on positional astronomy and celestial mechanics. Universitat de Valencia. 1998. p. 73-80

Author

Tsvetkov, A.S. / Kinematics of the Local Stellar system. Proceedings of the IV international workshop on positional astronomy and celestial mechanics. Universitat de Valencia, 1998. pp. 73-80

BibTeX

@inproceedings{c63b893a220740ffaedddfd822a15039,
title = "Kinematics of the Local Stellar system",
abstract = "The hypothesis of the rotation of the Local stellar system (LSS) is used to explain the components in the proper motions of stars that the standard kinematic model does not describe. The LSS rotational parameters are derived from the proper motions of the GC reduced onto fundamental systems of the catalogues N30, FK4 and FK5. A weak dependence of the parameters on choice of the fundamental system is found. Some preliminary results are obtained from the radial velocities of the FK5 and the proper motions of the PPM.",
keywords = "Local stellar system, Galactic rotation",
author = "A.S. Tsvetkov",
year = "1998",
language = "English",
pages = "73--80",
booktitle = "Proceedings of the IV international workshop on positional astronomy and celestial mechanics",
publisher = "Universitat de Valencia",
address = "Spain",

}

RIS

TY - GEN

T1 - Kinematics of the Local Stellar system

AU - Tsvetkov, A.S.

PY - 1998

Y1 - 1998

N2 - The hypothesis of the rotation of the Local stellar system (LSS) is used to explain the components in the proper motions of stars that the standard kinematic model does not describe. The LSS rotational parameters are derived from the proper motions of the GC reduced onto fundamental systems of the catalogues N30, FK4 and FK5. A weak dependence of the parameters on choice of the fundamental system is found. Some preliminary results are obtained from the radial velocities of the FK5 and the proper motions of the PPM.

AB - The hypothesis of the rotation of the Local stellar system (LSS) is used to explain the components in the proper motions of stars that the standard kinematic model does not describe. The LSS rotational parameters are derived from the proper motions of the GC reduced onto fundamental systems of the catalogues N30, FK4 and FK5. A weak dependence of the parameters on choice of the fundamental system is found. Some preliminary results are obtained from the radial velocities of the FK5 and the proper motions of the PPM.

KW - Local stellar system

KW - Galactic rotation

M3 - Conference contribution

SP - 73

EP - 80

BT - Proceedings of the IV international workshop on positional astronomy and celestial mechanics

PB - Universitat de Valencia

ER -

ID: 4482584