Hostname: page-component-7dd5485656-2pp2p Total loading time: 0 Render date: 2025-10-31T16:55:52.697Z Has data issue: false hasContentIssue false
  • English
  • Français

Dark Matter Problem in the Local Supercluster

Published online by Cambridge University Press:  01 June 2007

Dmitry Makarov  and
Igor Karachentsev
Dmitry Makarov
Affiliation:
Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskij region, Karachai-Cirkassian Republic, Russia 369167 email: dim@sao.ru
Igor Karachentsev
Affiliation:
Special Astrophysical Observatory of the Russian Academy of Sciences, Nizhnij Arkhyz, Zelenchukskij region, Karachai-Cirkassian Republic, Russia 369167 email: dim@sao.ru
Rights & Permissions [Opens in a new window]

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.

The Local Supercluster is an ideal laboratory to study distribution of luminous and dark matter in the nearby Universe. The 1100 small groups have been selected using algorithm based on assumption that a total energy of physical pair of galaxies must be negative. The properties of the groups have been considered.

Keywords

dark matter

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S244: Dark Galaxies and Lost Baryons , June 2007 , pp. 370 - 371
Copyright
Copyright © International Astronomical Union 2008

References

Bell, et al. 2003, ApJ 149, 289Google Scholar
Cole, et al. 2001, MNRAS 326, 255CrossRefGoogle Scholar
Heisler, et al. 1985, ApJ 298, 8CrossRefGoogle Scholar
Makarov, & Karachentsev, , 2000, ASPC 209, 40Google Scholar
Spergel, et al. 2007, ApJS 170, 377CrossRefGoogle Scholar