Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-27T00:38:51.690Z Has data issue: false hasContentIssue false
  • English
  • Français

High velocity clouds near the Magellanic Clouds

Published online by Cambridge University Press:  19 July 2016

Ulrich Mebold
Ulrich Mebold*
Affiliation:
Radioastronomisches Institut der Universität Bonn, Auf dem Hügel 71, D-5300 Bonn 1, Federal Republic of Germany

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.

High velocity clouds (HVCs) of neutral atomic hydrogen close to the position of the Magellanic Clouds (MCs) and the Magellanic Stream (Stream) are reviewed. The gas observed at velocities of +70 km/s and +130 km/s in front of the LMC is probably associated with ordinary HVCs in the galactic halo. This is not the case for the gas observed between +150 and +170 km/s which is more likely associated with the MCs. The HVCs observed superimposed onto the Stream are possibly remnants of collisions between a gaseous polar ring around our Galaxy and the bridge region between the MCs. The HVCs found close to and “behind” the tip of the Stream may be regarded as shreds of the Stream precipitating toward the galactic disk. The chemical composition, the radiation field and the temperature in the Stream is discussed in the context of the first spin temperature determination by Wakker (1990), of an HVC.

Type
The LMC-SMC-Galaxy System
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 463 - 468
Copyright
Copyright © Kluwer 1991 

References

de Boer, K.S., Morras, R. & Bajaja, E. (1990), Astron. Astrophys. 233, 523.Google Scholar
Cohen, R.J. (1981), Mon. Not. R. Astron. Soc. 196, 835.Google Scholar
Cohen, R.J. (1982), Mon. Not. R. Astron. Soc. 200, 391.Google Scholar
Cohen, R.J. & Mirabel, I.F. (1979), Mon. Not. R. Astron. Soc. 186, 217.CrossRefGoogle Scholar
Colgan, S.W.J., Salpeter, E.E. & Terzian, Y. (1990), Astrophys. J. 351, 503.CrossRefGoogle Scholar
Fong, R., Jones, L.R., Shanks, T., Stevenson, P.R.F., Strong, A.W., Dawe, J.A. & Murray, J.D. (1987), Mon. Not. Astron. Soc. 224, 1059.Google Scholar
Franco, J., Tenorio-Tagle, G., Bodenheimer, P., Rozyczka, M. & Mirabel, I.F. (1988), Astrophys.J. 333, 826.Google Scholar
Giovanelli, R., Verschuur, G.L. & Cram, T.R. (1973, Astron. Astrophys. Suppl. 12, 209.Google Scholar
Giovanelli, R. (1981), Astron. J. , 86, 1468.Google Scholar
Giovanelli, R. (1986), Gaseous Halos of Galaxies, NRAO Workshop No. 12 , Green Bank, W.Va., Bregman, J.N. & Lockman, F.J. (eds) p.99.Google Scholar
Giovanelli, R. & Haynes, M.P. (1976), Mon. Not. R. Astron. Soc. 177, 525.CrossRefGoogle Scholar
Haud, U. (1988), Astron. Astrophys. , 198, 125.Google Scholar
Haynes, M.P. (1979), Astron. J. 84, 1173.CrossRefGoogle Scholar
Heiles, C. (1984), Astrophys. J. Suppl. 55, 585.CrossRefGoogle Scholar
Mathewson, D.S., Cleary, M.N. & Murray, J.D. (1974), Astrophys.J. 190, 291.CrossRefGoogle Scholar
Mathewson, D.S., Cleary, M.N., Murray, J.D. (1975), Astrophys.J. 195, L97.CrossRefGoogle Scholar
Mathewson, D.S., Wayte, S.R., Ford, V.L. & Ruan, K. (1987), Proc. Astron. Soc. Austr. 7, 19.CrossRefGoogle Scholar
McGee, R.X., Newton, L.M. & Morton, D.C. (1983), Mon. Not. R. Astron. Soc. 205, 1191.CrossRefGoogle Scholar
Mebold, U., de Boer, K.S., Wennmacker, A. (1990), Proc. 11th Europ. Reg. Astron. Meeting , Tenerifa, in press.Google Scholar
Mebold, U., Herbstmeier, U., Kalberla, P.M.W. & Souvatzis, I. (1989), Structure and Dynamics of the Interstellar Medium , Tenorio-Tagle, G. et al. (eds), IAU Coll. 120 in press.Google Scholar
Mirabel, I.F. (1982), Astrophys. J. 256, 112.CrossRefGoogle Scholar
Mirabel, I.F., Cohen, R.J. & Davies, R.D. (1979), Mon. Not. R. Astron. Soc. 186, 433.CrossRefGoogle Scholar
Morras, R. (1983), Astron. J. 88, 62.ß.Google Scholar
Morras, R. (1985), Astron. J. 90, 1801.Google Scholar
Payne, H.E., Salpeter, E.E. & Terzian, Y. (1980), Astrophys. J. 240, 499.Google Scholar
Penston, M.V. (1982, The Observatory 102, 174.Google Scholar
Rohlfs, R., Herbstmeier, U., Mebold, U. & Winnberg, A. (1989), Astron. Astrophys. 211, 402.Google Scholar
Songaila, A. (1981), Astrophys. J. 243, L19.Google Scholar
de Vaucouleurs, G. (1955), Astron. J. 60, 126.Google Scholar
de Vaucouleurs, G. & Freeman, K.C. (1972), Vistas Astron. 14, 163.Google Scholar
Wakker, B. (1990), Ph.D. Thesis, Univ. Groningen.Google Scholar
Wayte, S.R. (1990a), Astrophys. J. 355, 473.Google Scholar
Wayte, S.R. (1990b), this volume.Google Scholar
Wesselius, P.R. & Fejes, I. (1973), Astron. Astrophys. 24, 15.Google Scholar
West, K.A., Pettini, M., Penston, M.V., Blades, J.C. & Morton, D.C. (1985), Mon. Not. R. Astron. Soc. 215, 481.Google Scholar
Van Woerden, H., Schwarz, U.J. & Hulsbosch, A.N.M. (1985) IAU Symposium 106, The Milky Way Galaxy , van Woerden, et al. (eds) (Reidel: Dordrecht) p.387.Google Scholar
Van Woerden, H., Schwarz, U.J., Robertson, J.G. & Hulsbosch, A.N.M. (1986), Gaseous Halos of Galaxies, NRAO Workshop No. 12 , Green Bank, W.Va, Bregman, J.N. & Lockman, F.J., (eds) p.115.Google Scholar