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The Local star system: Kinematics derived from radial velocities. / Tsvetkov, A.S.

In: Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, Vol. 8, 1995, p. 145-156.

Research output: Contribution to journal › Article

Harvard

Tsvetkov, AS 1995, 'The Local star system: Kinematics derived from radial velocities', Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, vol. 8, pp. 145-156. https://doi.org/10.1080/10556799508203302

APA

Tsvetkov, A. S. (1995). The Local star system: Kinematics derived from radial velocities. Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society, 8, 145-156. https://doi.org/10.1080/10556799508203302

Vancouver

Tsvetkov AS. The Local star system: Kinematics derived from radial velocities. Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society. 1995;8:145-156. https://doi.org/10.1080/10556799508203302

Author

Tsvetkov, A.S. / The Local star system: Kinematics derived from radial velocities. In: Astronomical and Astrophysical Transactions. Journal of the Eurasian Astronomical Society. 1995 ; Vol. 8. pp. 145-156.

BibTeX

@article{0b2201101e0f4f4daf47c43dd7d21794,
title = "The Local star system: Kinematics derived from radial velocities",
abstract = "The rotational parameten, of the Local star system have been derived from radial velocities of 2537 stars of FK5. The most likely geometrical description of the Local system is presented. The results obtained from the radial velocities do not contradict those derived from proper motions and may be considered as evidence for the existence of the Local Star system.",
keywords = "Radial velocities, local star system",
author = "A.S. Tsvetkov",
year = "1995",
doi = "10.1080/10556799508203302",
language = "English",
volume = "8",
pages = "145--156",
journal = "Astronomical and Astrophysical Transactions",
issn = "1055-6796",
publisher = "Cambridge Scientific Publishers",

}

RIS

TY - JOUR

T1 - The Local star system: Kinematics derived from radial velocities

AU - Tsvetkov, A.S.

PY - 1995

Y1 - 1995

N2 - The rotational parameten, of the Local star system have been derived from radial velocities of 2537 stars of FK5. The most likely geometrical description of the Local system is presented. The results obtained from the radial velocities do not contradict those derived from proper motions and may be considered as evidence for the existence of the Local Star system.

AB - The rotational parameten, of the Local star system have been derived from radial velocities of 2537 stars of FK5. The most likely geometrical description of the Local system is presented. The results obtained from the radial velocities do not contradict those derived from proper motions and may be considered as evidence for the existence of the Local Star system.

KW - Radial velocities

KW - local star system

U2 - 10.1080/10556799508203302

DO - 10.1080/10556799508203302

M3 - Article

VL - 8

SP - 145

EP - 156

JO - Astronomical and Astrophysical Transactions

JF - Astronomical and Astrophysical Transactions

SN - 1055-6796

ER -

ID: 5202600