No CrossRef data available.
Article contents
Interaction of Disks and Dark Haloes of Dwarf Spirals
Published online by Cambridge University Press: 25 May 2016
Extract
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.
In a number of dwarf spiral galaxies the HI-emission has been studied with sufficient resolution to derive the rotation curves of the galaxies. These show that the disks of dwarf spirals are imbedded in extended haloes of dark matter, quite similar to the disks of giant spiral galaxies.
- Type
- Dark Matter Halos around Galaxies
- Information
- Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 171 - 174
- Copyright
- Copyright © Kluwer 1996
References
Toomre, A.
1981, in The Structure and Evolution of Normal Galaxies, eds. Fall, S. M. & Lynden-Bell, D. (Cambridge: Cambridge Univ. Press) p.111
Google Scholar
Wielen, R., & Fuchs, B.
1983, in Kinematics, Dynamics and Structure of the Milky Way, ed Shuter, W. L. H. (Dordrecht: Reidel) p.81
Google Scholar
Wielen, R., Dettbarn, C., Fuchs, B., Jahreiß, H., & Radons, G.
1992, IAU Symp. No. 149, p.81
Google Scholar