Skip to main content
SpringerLink
Log in

Dark Matter in Wide Triple Systems of Galaxies

  • Published:
Astrophysics and Space Science Aims and scope Submit manuscript

Abstract

Numerical models for wide triplets of galaxies are developed, and a statistical estimate of the dark matter content in these systems is derived. In a typical system, the mass of dark matter proves to be (1.5 - 3) × 1012h-1 M⊙.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  • Chernin, A.D. and Mikkola, S.: 1991, MN RAS 253, 153

    Google Scholar 

  • Trofimov, A.V. and Chernin, A.D.: 1995, Astron. Rep. 72No.3

Download references

Author information

Authors and Affiliations

  1. Sternberg Astronomical Institute, Moscow University, Moscow, 119899, Russia

    Valentin P. Dolgachev & Arthur D. Chernin

Authors
  1. Valentin P. Dolgachev
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. Arthur D. Chernin
    View author publications

    You can also search for this author in PubMed Google Scholar

Rights and permissions

Reprints and permissions

About this article

Cite this article

Dolgachev, V.P., Chernin, A.D. Dark Matter in Wide Triple Systems of Galaxies. Astrophysics and Space Science 252, 151–153 (1997). https://doi.org/10.1023/A:1000870300913

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1023/A:1000870300913

Keywords

Search

Navigation