A new approach to the construction of stellar velocity field in the Sun's neighborhood

Research output

Abstract

The new method to construct the three-dimensional stellar velocity field is discussed.It is shown that it is not necessary to have the radial velocities if the parallax of each star is known.
Original languageEnglish
Title of host publicationProc. of the Conference "Stellar dynamics: from classic to modern"
Publication statusPublished - 2001

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parallax
radial velocity
sun
velocity distribution
stars

Cite this

Tsvetkov, A. S. (2001). A new approach to the construction of stellar velocity field in the Sun's neighborhood. In Proc. of the Conference "Stellar dynamics: from classic to modern"
Tsvetkov, A.S. / A new approach to the construction of stellar velocity field in the Sun's neighborhood. Proc. of the Conference "Stellar dynamics: from classic to modern". 2001.
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abstract = "The new method to construct the three-dimensional stellar velocity field is discussed.It is shown that it is not necessary to have the radial velocities if the parallax of each star is known.",
keywords = "Hipparocs, Stellar kinematics",
author = "A.S Tsvetkov",
year = "2001",
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booktitle = "Proc. of the Conference {"}Stellar dynamics: from classic to modern{"}",

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Tsvetkov, AS 2001, A new approach to the construction of stellar velocity field in the Sun's neighborhood. in Proc. of the Conference "Stellar dynamics: from classic to modern".

A new approach to the construction of stellar velocity field in the Sun's neighborhood. / Tsvetkov, A.S.

Proc. of the Conference "Stellar dynamics: from classic to modern". 2001.

Research output

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T1 - A new approach to the construction of stellar velocity field in the Sun's neighborhood

AU - Tsvetkov, A.S

PY - 2001

Y1 - 2001

N2 - The new method to construct the three-dimensional stellar velocity field is discussed.It is shown that it is not necessary to have the radial velocities if the parallax of each star is known.

AB - The new method to construct the three-dimensional stellar velocity field is discussed.It is shown that it is not necessary to have the radial velocities if the parallax of each star is known.

KW - Hipparocs

KW - Stellar kinematics

M3 - Article in an anthology

BT - Proc. of the Conference "Stellar dynamics: from classic to modern"

ER -

Tsvetkov AS. A new approach to the construction of stellar velocity field in the Sun's neighborhood. In Proc. of the Conference "Stellar dynamics: from classic to modern". 2001