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.
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Silich, S.A. Three-dimensional supershells in differentially-rotating galactic disks. Astrophys Space Sci 195, 317–330 (1992). https://doi.org/10.1007/BF00646764
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DOI: https://doi.org/10.1007/BF00646764