Hostname: page-component-78c5997874-t5tsf Total loading time: 0 Render date: 2024-11-16T05:11:27.520Z Has data issue: false hasContentIssue false
  • English
  • Français

Mass Distribution and Dark Halos

Published online by Cambridge University Press:  04 August 2017

U. Haud  and
J. Einasto
U. Haud
Affiliation:
Tartu Astrophysical Observatory
J. Einasto
Affiliation:
Tartu Astrophysical Observatory

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.

One of the most controversial astronomical paradoxes seems to be the mass paradox : the mass of large astronomical systems depends on the mass determination method. This paradox can be explained by supposing the existence of huge invisible coronas of unknown origin around galaxies. In the present paper we discuss basic empirical evidence of hidden matter in galaxies and examine the total mass distribution.

Type
I. Kinematics of Gas and the Underlying Mass Distribution
Information
Symposium - International Astronomical Union , Volume 100: Internal Kinematics and Dynamics of Galaxies , 1983 , pp. 81 - 88
Copyright
Copyright © Reidel 1983 

References

Bahcall, J.N. and Sarrazin, C.L.: 1977, Astrophys. J. 213, L99.Google Scholar
Bosma, A.: 1978, Dissertation, University of Groningen.Google Scholar
Davies, M. et al. : 1980, Astrophys. J. 238, L113.Google Scholar
Einasto, J.: 1972, Proc. First European Astr. Meeting 2, 291.Google Scholar
Einasto, J., Kaasik, A. and Saar, E.: 1974a, Nature 250, 309.Google Scholar
Einasto, J., et al.: 1974b, Tartu Astron. Obs. Teated 48, 3.Google Scholar
Einasto, J., et al.: 1976, Mon. Not. R. astr. Soc. 177, 357.Google Scholar
Einasto, J., Joeveer, M. and Saar, E.: 1979, Tartu Astron. Obs. Preprint A-2.Google Scholar
Einasto, J. and Kaasik, A.: 1982, Tartu Astron. Obs. Preprint.Google Scholar
Einasto, J. and Lynden-Bell, D.: 1982, Mon. Not. R. astr. Soc. 199, 67.Google Scholar
Faber, S. and Gallagher, J.: 1979, Ann. Rew. Astron. Astrophys. 17, 135.Google Scholar
Fabricant, D., Lecar, J. and Gorenstein, P.: 1980, Astrophys. J. 241, 552.Google Scholar
Gott, J.R. III and Thuan, T.X.: 1978, Astrophys. J. 223, 426.CrossRefGoogle Scholar
Hartwick, F.D.A. and Sargent, W.L.W.: 1978, Astrophys. J. 221, 512.Google Scholar
Haud, U.: 1981, Astrophys. Space Sci. 76, 477.Google Scholar
Jaaniste, J. and Saar, E.: 1976, Tartu Astrophys. Obs. Publ. 43, 216.Google Scholar
Lynden-Bell, D.: 1976, Mon. Not. R. astr. Soc. 174, 695.Google Scholar
Lynden-Bell, D.: 1981, Observatory 101, 111.Google Scholar
Mitchell, R. and Mushotzky, R.: 1980, Astrophys. J. 236, 730.Google Scholar
Ostriker, J.P., Peebles, P.J.E. and Yahil, A.: 1974, Astrophys. J. 193, L1.Google Scholar
Peebles, P.J.E.: 1980, The Large-scale Structure of the Universe, Princeton University Press, Princeton, New Jersey.Google Scholar
Takahara, M. and Takahara, F.: 1980, Kyoto Univ. Preprint 405, 1.Google Scholar
Vaucouleurs, G. de: 1953, Mon. Not. R. astr. Soc. 113, 134.CrossRefGoogle Scholar