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A study of the properties of galactocentric orbits

Published online by Cambridge University Press:  07 August 2017

A. A. Myullyari ,
Yu. V. Nechitajlov ,
S. Ninković  and
V. V. Orlov
A. A. Myullyari
Affiliation:
University of Petrozavodsk, USSR
Yu. V. Nechitajlov
Affiliation:
St Petersburg State University, 198904 Petrodvorets, Bibliotechnaya ploshchad' 2, USSR
S. Ninković
Affiliation:
Astronomical Observatory, Volgina 7, 11050 Beograd, Yugoslavia
V. V. Orlov
Affiliation:
St Petersburg State University, 198904 Petrodvorets, Bibliotechnaya ploshchad' 2, USSR

Abstract

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The galactocentric motion of 14 stars from the solar neighbourhood is studied. The stars are divided into nine groups according to their heliocentric-velocity components. In this way one can follow the motion of the stars belonging to the same group in the past.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 461
Copyright
Copyright © Kluwer 

References

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