Skip to main content
Log in

Application of a tensor virial equation for the determination of the possible figures of self-gravitating matter in the presence of a magnetic field

  • Published:
Astrophysics Aims and scope

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

Access this article

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

Instant access to the full article PDF.

Literature Cited

  1. S. P. S. Anand and R. S. Kushwaha, Ann. Astrophys.,25, 310 (1962).

    Google Scholar 

  2. I. W. Roxburgh and B. R. Durney, M. N.,135, 329 (1967).

    Google Scholar 

  3. N. R. Lebovitz, Ap. J.,134, 500 (1961).

    Google Scholar 

  4. R. S. Oganesyan and M. G. Abramyan, Astron. Zh. (in press).

  5. M. F. Subbotin, Course of Celestial Mechanics [in Russian], Vol. 3, Gostekhizdat, Moscow (1949).

    Google Scholar 

  6. G. A. Gurzadyan, Planetary Nebulae [in Russian], Fizmatgiz, Moscow (1962).

    Google Scholar 

  7. T. A. Lozinskaya, Astron. Zh.,49, 1158 (1972).

    Google Scholar 

Download references

Authors

Additional information

Erevan State University. Translated from Astrofizika, Vol. 9, No. 3, pp. 401–416, July–September, 1973.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Oganesyan, R.S., Abramyan, M.G. Application of a tensor virial equation for the determination of the possible figures of self-gravitating matter in the presence of a magnetic field. Astrophysics 9, 230–240 (1973). https://doi.org/10.1007/BF01007188

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF01007188

Keywords

Navigation