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Mass Distribution and Dark Halos

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Part of the book series: International Astronomical Union/Union Astronomique Internationale ((IAUS,volume 100))

Abstract

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.

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© 1983 IAU

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Haud, U., Einasto, J. (1983). Mass Distribution and Dark Halos. In: Athanassoula, E. (eds) Internal Kinematics and Dynamics of Galaxies. International Astronomical Union/Union Astronomique Internationale, vol 100. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7075-5_20

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  • DOI: https://doi.org/10.1007/978-94-009-7075-5_20

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-277-1547-0

  • Online ISBN: 978-94-009-7075-5

  • eBook Packages: Springer Book Archive

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