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The Magellanic Stream: New Observations

Published online by Cambridge University Press:  25 April 2016

S. R. Wayte
S. R. Wayte*
Affiliation:
Mount Stromlo and Siding Spring Observatories, The Australian National University
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Abstract

New HI observations of the Magellanic Stream have been made using the Parkes 64 m telescope. These observations highlight in detail its complicated structure and uncover new features of the Stream. The extreme velocity clouds (EVCs) are morphologically linked to the Stream indicating that these HI clouds are very likely truly part of the Stream. Also it is suggested that many of the high velocity clouds seen around the Stream are indeed part of the Magellanic Stream itself, and that the stream consists of many different velocity components in bulk motion.

Type
Miscellaneous Radio Astronomy
Information
Publications of the Astronomical Society of Australia , Volume 8 , Issue 2 , 1989 , pp. 195 - 203
Copyright
Copyright © Astronomical Society of Australia 1989

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References

Brück, M. T. and Hawkins, M. R. S., 1983, Astron. Astrophys., 124, 216.Google Scholar
Feitzinger, J. V., Isserstedt, J. and Schmidt-Kaler, Th., 1977, Astron. Astrophys., 57, 265.Google Scholar
Green, H. E., 1980a, Proc. Astron. Soc.Aust., 4, 30.Google Scholar
Green, H. E., 1980b, ‘Experimental Determination of the Radiation Diagram of the Parkes Radio Telescope using a Geostationary Satellite’, CSIRO Division of Radiophysics Internal Report RPP 2420.Google Scholar
Harten, R. H., Westerhout, G. and Kerr, F. J., 1975, Astron. J., 80, 307.Google Scholar
Huslsbosch, A. N. M. and Wakker, B.P., 1988, Submitted to Astron. Astrophys. Supp. Series.Google Scholar
Kalberla, P. M. W., Mebold, U. and Reif, K., 1982, Astron. Astrophys., 106, 190.Google Scholar
Mathewson, D. S. and Ford, V. L., 1984, ‘Structure and Evolution of the Magellanic Clouds’, IAU Symp. No. 108, ed. Van Den Bergh, S. and De Boer, K. S., (Dordrecht: Reidel), p. 125.Google Scholar
Mathewson, D. S., Ford, V. L., Schwarz, M. P. and Murray, J. D., 1979, ‘The Large Scale Characteristics of the Galaxy’, IAU Symp. No. 84, ed. Burton, W. B., (Dordrecht: Reidel), p. 547.Google Scholar
Mathewson, D.S., Schwarz, M. P. and Murray, J. D., 1977, Astrophys. J. Lett., 217, L5.CrossRefGoogle Scholar
Mathewson, D. S., Wayte, S. R., Ford, V. L. and Ruan, K., 1987, Proc. Astron. Soc. Aust., 7, 19.Google Scholar
Meatheringham, S. J. and Dopita, M. A., 1986, Proc. Astron. Soc. Aust., 6, 464.Google Scholar
Mirabel, I. F., 1981, Astrophys. J., 250, 528.CrossRefGoogle Scholar
Morras, R., 1983, Astron. J., 88, 62.Google Scholar
Morras, R., 1985, Astron. J., 90, 1801.Google Scholar
Wright, M. C. H., 1974, Astron. Astrophys., 31, 317.Google Scholar
Wright, M. C. H., 1979a, Astrophys. J., 233, 35.Google Scholar
Wright, M.C. H., 1979b, Astrophys. J., 234, 27.Google Scholar