Hostname: page-component-77c89778f8-cnmwb Total loading time: 0 Render date: 2024-07-16T17:24:46.808Z Has data issue: false hasContentIssue false
  • English
  • Français

Galactic rotation and velocity fields

Published online by Cambridge University Press:  04 August 2017

W.L.H. Shuter  and
A. Gill
W.L.H. Shuter
Affiliation:
University of British Columbia
A. Gill
Affiliation:
University of British Columbia

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.

Using unpublished 21-cm data from Jackson and Kerr of the entire Galaxy at b = 0°, we have determined the terminal velocities, vm, to be (Gill & Shuter, 1983)

Type
PART II: COMPOSITION, STRUCTURE AND KINEMATICS
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 109 - 110
Copyright
Copyright © Reidel 1985 

References

Gill, A., & Shuter, W.L.H.: 1983, MNRAS, in press.Google Scholar
Gunn, J.E., Knapp, G.R., & Tremaine, S.D.: 1979, Astron. J., 84, 1181 Google Scholar
Ovenden, M.W., Pryce, M.H.L., & Shuter, W.L.H.: 1983 in “Kinematics, Dynamics and Structure of the Milky Way”, ed. Shuter, W.L.H., (Dordrecht, Holland : Reidel), p. 67–72.CrossRefGoogle Scholar