Skip to main content
SpringerLink
Log in

Relativistic magnetic partially degenerate isothermal gas spheres

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

Abstract

The effect of a poloidal magnetic field on the structure of isothermal gas spheres in hydrostatic equilibrium under the pressure of partially degenerate relativistic electrons and radiation has been considered. An equation of state involving Fermi-Dirac functionsF 2(ψ) andF 3(ψ) has been used. Modifications to the values of various structural parameters have been tabulated for the cases ψ c =0, 2, 3, 5, and 10, ψ c being the central degeneracy parameter.

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

Download references

Author information

Authors and Affiliations

  1. Institut für Reine und Angewandte Kernphysik, Abteilung Mathematische Physik, Universität Kiel, Germany

    Harinder Pal Singh (Deutscher Akademischer Austauschdienst (DAAD) Fellow)

Authors
  1. Harinder Pal Singh
    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

Pal Singh, H. Relativistic magnetic partially degenerate isothermal gas spheres. Astrophys Space Sci 184, 143–146 (1991). https://doi.org/10.1007/BF00644870

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00644870

Keywords

Search

Navigation