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The Magellanic Stream: theoretical considerations

Published online by Cambridge University Press:  14 August 2015

M. Fujimoto
M. Fujimoto*
Affiliation:
Department of Physics Nagoya University, Nagoya

Abstract

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The tidal and the primordial theories for the Magellanic Stream are examined in a frame of test-particle simulation for the interacting triple system of the Galaxy, the Large and Small Magellanic Clouds (LMC and SMC). Difficulties of the radial velocity of the Stream still beset these two theories. Several new models for the Stream and the Clouds are briefly discussed in relation to the bending of the galactic disk, the past binary orbits of the LMC and SMC and also the Local Group and the Local Supercluster of galaxies.

Type
X. HIGH-VELOCITY CLOUDS AND THE MAGELLANIC STREAMS
Information
Symposium - International Astronomical Union , Volume 84: The Large-Scale Characteristics of the Galaxy , 1979 , pp. 557 - 566
Copyright
Copyright © Reidel 1979 

References

Davies, R.D. and Wright, A.E.: 1977, Mon. Not. R. astr. Soc. 180, pp.71–88.Google Scholar
de Vaucouleurs, G. and Corwin, H.G.: 1975, Astrophys. J. 202, pp.327–334.Google Scholar
Hindman, J.V., Kerr, F.J., and McGee, R.X.: 1963, Australian J. Phys. 16, pp.570–883.Google Scholar
Hunter, C. and Toomre, A.: 1969, Astrophys. J. 155, pp.747–776.CrossRefGoogle Scholar
Fujimoto, M. and Sofue, Y.: 1966, Astron. Astrophys. 47, pp.263–291.Google Scholar
Fujimoto, M. and Sofue, Y.: 1977, Astron. Astrophys. 61, pp.199–215.Google Scholar
Lynden-Bell, D.: 1976, Mon. Not. R. astr. Soc. 174, pp.695–710.CrossRefGoogle Scholar
Mathewson, D.S. and Ford, V.L.: 1970, Astrophys. J. (Letters) 160, pp.43–46.Google Scholar
Mathewson, D.S., Cleary, U.N., and Murray, J.C.: 1974, Astrophys. J. 190, pp.291–296.CrossRefGoogle Scholar
Mathewson, D.S. and Schwarz, M.P.: 1976, Mon. Not. R. astr. Soc. 176, 47P–51P.Google Scholar
Mathewson, D.S., Schwarz, M.P., and Murray, J.D.: 1977, Astrophys. J. (Letters) 217, pp.5–8.Google Scholar
Mirabel, I.E. and Turner, K.C.: 1973, Astron. Astrophys. 22, pp.437–440.Google Scholar
Ostriker, J.P. and Peebles, P.J.E.: 1973, Astrophys. J. 186, pp.467–480.Google Scholar
Schmidt, Th.: 1970, Astron. Astrophys. 6, pp.294–308.Google Scholar
Spight, L. and Crayzeck, E.: 1977, Astrophys. J. 213, pp.374–378.Google Scholar
Toomre, A. and Toomre, J.: 1972, Astrophys. J. 178, pp.623–666.Google Scholar
Toomre, A.: 1973, in Mirabel and Turner (1973) given above.Google Scholar
Tremaine, S.D.: 1976, Astrophys. J. 203, pp.72–74.Google Scholar
van Kuilenberg, J.: 1972, Astron. Astrophys. 16, pp.276–281.Google Scholar
Wannier, P. and Wrixon, G.T.: 1972, Astrophys. J. (Letter) 173, pp.119–123.Google Scholar