A gaseous shock wave theory of the galactic spiral structure

DOI10.1007/BF01877656zbMath0543.76093OpenAlexW2067975746MaRDI QIDQ796398

Wen-rui Hu

Publication date: 1982

Published in: Applied Mathematics and Mechanics. (English Edition) (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01877656

zbMATH Keywords

iterative methodself-gravitationgalactic spiral structureinterstellar gaslocal shockmass distribution in proto-galactic disk

Mathematics Subject Classification ID

Shock waves and blast waves in fluid mechanics (76L05) Galactic and stellar dynamics (85A05)

Related Items (1)

High speed flows and shock waves in astrophysical problems

Cites Work

• On the Distribution of Matter Within Highly Flattened Galaxies.

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