Hostname: page-component-77c89778f8-vsgnj Total loading time: 0 Render date: 2024-07-19T08:15:45.002Z Has data issue: false hasContentIssue false

The kinematics of nearby stars and large-scale radial motion in the Galaxy

Published online by Cambridge University Press:  04 August 2017

S.V.M. Clube*
Affiliation:
Royal Observatory, Edinburgh, Scotland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The concept of star streams originally due to Kapteyn is revived. It is suggested that the existence of Stream II may have been overlooked, yet it is of crucial importance in specifying the true local standard of rest.

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Copyright
Copyright © Reidel 1985 

References

Bania, T.M.: 1985, these Proceedings, Section II.3 Google Scholar
Blaauw, A.: 1985, these Proceedings, Section II.6 Google Scholar
Clube, S.V.M.: 1978, M.N.R.A.S. 184, 553 CrossRefGoogle Scholar
Clube, S.V.M., and Watson, F.G.: 1979, M.N.R.A.S. 187, 863 CrossRefGoogle Scholar
Clube, S.V.M., Watson, F.G., and Zhao, J.L.: 1983, Astron. Astrophys. in press Google Scholar
Eddington, A.S.: 1914, Stellar Movements and the Structure of the Universe, London: MacMillan Google Scholar
Eggen, O.J.: 1963, Astron. J. 68, 697 CrossRefGoogle Scholar
Griffin, R.F., Zhao, J.L., and Clube, S.V.M.: 1983, in preparation Google Scholar
Kinman, T.D.: 1959, M.N.R.A.S. 119, 559 CrossRefGoogle Scholar
Upgren, A.R.: 1976, Bull. Amer. astr. Soc. 8, 4, 542 Google Scholar
Woolley, R.v.d.R. et al.: 1977, M.N.R.A.S. 179, 81 CrossRefGoogle Scholar