Hostname: page-component-7857688df4-vhqbq Total loading time: 0 Render date: 2025-11-18T00:59:50.506Z Has data issue: false hasContentIssue false
  • English
  • Français

The Magellanic Stream: the Turbulent Wake of the Magellanic Clouds in the Halo of the Galaxy

Published online by Cambridge University Press:  25 April 2016

D. S. Mathewson ,
M. P. Schwarz  and
J. D. Murray
D. S. Mathewson
Affiliation:
Mount stromlo and Siding Spring Observatory, Australian National University
M. P. Schwarz
Affiliation:
Mount stromlo and Siding Spring Observatory, Australian National University
J. D. Murray
Affiliation:
Division of Radiophysics, CSIRO, Sydney
Get access Rights & Permissions [Opens in a new window]

Extract

New observations of the Magellanic Stream were made in December 1976 with the 64-m radio telescope at the Parkes Observatory of CSIRO. The ridges of H I emission of the Stream were traced from near its tip at ℓ = 90°, b = -40° to the Magellanic Clouds. This was the first time that the total length of the Stream was observed with the one system (only possible from the southern hemisphere) and with high spatial (15’ of arc) and velocity (4 km s-1) resolution. The results of this survey are presented in Figures 1 and 2 and the main features are listed below.

Information

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 3 , Issue 2 , September 1977 , pp. 133 - 136
Copyright
Copyright © Astronomical Society of Australia 1977

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Article purchase

Temporarily unavailable

References

Davies, R. D., and Wright, A. E., Mon. Not. R. Astr. Soc, (in press) (1977).Google Scholar
Field, G. B., Astrophys. J., 142, 531 (1965).Google Scholar
Fujimoto, M., and Sofue, Y., Astron. and Astrophys., 47, 263 (1976).Google Scholar
Fujimoto, M., and Sofue, Y., Astron. and Astrophys., (in press) (1977).Google Scholar
Goldstein, S., Modern Developments in Fluid Dynamics, Dover Publications Inc., New York (1965).Google Scholar
Lynden-Bell, D., Mon. Not. R. Astr. Soc, 174, 695 (1976).Google Scholar
Mathewson, D. S., Cleary, M. N., and Murray, J. D., Astrophys. J., 190, 291 (1974).Google Scholar
Mathewson, D. S., R. Greenwich Obs. Bull. No. 182 (1976).Google Scholar
Mathewson, D. S., and Schwarz, M. P., Mon. Not. R. Astr. Soc, 176, 47P (1976).Google Scholar
Shapiro, P. R., and Moore, R. T., Astrophys. J., 207, 460 (1976).Google Scholar
Silk, J., Comments on Ap. and Sp. Phys., 6, Part C, 1 (1974).Google Scholar
Townsend, A. A., The Structure of Turbulent Shear Flow, Cambridge Univ. Press, Cambridge (1976).Google Scholar
Wannier, P., and Wrixon, G. T., Astrophys. J. Lett., 173, L119 (1972).Google Scholar