Three-dimensional supershells in differentially-rotating galactic disks

Details Three-dimensional supershells in differentially-rotating galactic disks Three-dimensional supershells in differentially-rotating galactic disks

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.195..317s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 195, no. 2, p. 317-330.

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30

Galactic Structure, Interstellar Gas, Rotating Disks, Supernova Remnants, Computational Astrophysics, Galactic Rotation, Milky Way Galaxy

Scientific paper

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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