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Article contents
Possible influence of the galactic spiral structure on the local distributions of stellar residual velocities
Published online by Cambridge University Press: 14 August 2015
Extract
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