Astrophysics and Space Science

, Volume 195, Issue 2, pp 317–330 | Cite as

Three-dimensional supershells in differentially-rotating galactic disks

  • S. A. Silich
Article
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Abstract

The evolution of remnants produced by the correlated supernovae explosions in OB-associations is investigated. The 2.5-dimensional numerical hydrodynamic scheme based on thin layer approximation is proposed. Inhomogeneity of the gas density distribution, galactic disk shear, gravity, and continuous energy input from SNe explosions are taken into account.

Keywords

Thin Layer Density Distribution Energy Input Supernova Explosion Galactic Disk 
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Copyright information

© Kluwer Academic Publishers 1992

Authors and Affiliations

  • S. A. Silich
    • 1
  1. 1.Main Astronomical Observatory of the Ukrainian Academy of SciencesKievUkrainia

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