Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-14T05:46:10.010Z Has data issue: false hasContentIssue false
  • English
  • Français

Possible influence of the galactic spiral structure on the local distributions of stellar residual velocities

Published online by Cambridge University Press:  14 August 2015

M. Mayor
M. Mayor*
Affiliation:
Observatoire de Genève, Genève, Switzerland

Extract

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 residual velocity distribution, observed in the solar neighbourhood, exhibits several peculiarities for the stars of low epicyclic energy: vertex deviation, two-stream distribution, etc.

Type
Part IV/Comparison of Theory and Observations
Information
Symposium - International Astronomical Union , Volume 38: The Spiral Structure of our Galaxy , 1970 , pp. 433 - 434
Copyright
Copyright © Reidel 1970 

References

Lin, C. C.: 1967, in Relativity Theory and Astrophysics, 2 Galactic Structure Amer. Math. Soc., Providence, p. 66.Google Scholar
Lin, C. C. and Shu, F. H.: 1964, Astrophys. J. 140, 646.Google Scholar
Lin, C. C., Yuan, C., and Shu, F. H.: 1969, Astrophys. J. 155, 721.CrossRefGoogle Scholar