Log in

Possible evidence for a massive black hole in a quasar with double redshift systems

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

Abstract

With the aid of a simple black hole model of quasars we have found that the majority of the distinguishable emission lines in the spectrum of the quasar 1604+179 can be assigned to two redshift systems,z r =3.712 andz b =2.701. The appearance of double emission redshifts means that this quasar might be a massive black hole (of mass 108 M M≤1011 M ) with a ring-like emission line region (of radius 1 light-day ≤r 0≤1 light-year) in its accretion disk.

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

Access this article

Subscribe and save

Springer+ Basic
EUR 32.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or Ebook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

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

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Burbidge, E. M., Smith, H. E., Junkkarinen, V. S., and Hoag, A. A.: 1985,Astrophys. J. 288, 82.

    Google Scholar 

  • Deng Tieru: 1985, in preparation.

  • Fang Lizhi and Deng Tieru: 1982,Acta Physica Sinica 1, 110.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Liu, YZ., Deng, ZG., Zhou, YY. et al. Possible evidence for a massive black hole in a quasar with double redshift systems. Astrophys Space Sci 123, 137–144 (1986). https://doi.org/10.1007/BF00649129

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00649129

Keywords

Navigation