Skip to main content
Log in

An exact similarity solution for a spherical shock wave in a self-gravitating system

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

Abstract

In this paper we have obtained a similarity solution for a spherical magneto-gas dynamic shock wave in a self-gravitating system. It is observed that the total energy of the shock wave is not a constant, but it decreases with time. A remarkable change in radiation flux is also being observed here because of the presence of the magnetic field while there is no change in density, velocity and pressure.

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.

Similar content being viewed by others

References

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Srivastava, S.K., Singh, R.K. An exact similarity solution for a spherical shock wave in a self-gravitating system. Astrophys Space Sci 92, 365–372 (1983). https://doi.org/10.1007/BF00651301

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00651301

Keywords

Navigation