Galactic spiral shocks in a corrugated gas disc

Details Galactic spiral shocks in a corrugated gas disc Galactic spiral shocks in a corrugated gas disc

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210..381n&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Sept. 15, 1984, p. 381-392.

Statistics

Computation

3

Density Wave Model, Galactic Evolution, Galactic Structure, Interstellar Gas, Shock Waves, Spiral Galaxies, Computational Astrophysics, Disk Galaxies, Gas Density

Scientific paper

The interaction between a stellar density wave driven spiral shock and a
corrugation wave in a galactic disc is calculated numerically under the
tightly wound approximation. The results show that the detailed
structure of the galactic shock can be significantly modified by even a
small amplitude corrugation wave.

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