Gas flow in and around bars

Details Gas flow in and around bars Gas flow in and around bars

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..341a&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 341-348 (SEE N89-24910 18-75)

Astronomy and Astrophysics

Astrophysics

1

Barred Galaxies, Gas Flow, Interstellar Gas, Astronomical Models, Cosmic Dust, Flow Distribution, Flux Vector Splitting, Plasma Resonance

Scientific paper

The flow of gas in and around barred galaxies is calculated using a second order flux splitting code. For appropriate bar models shocks form along the leading edges of the bar, at positions where dust lanes are observed in barred galaxies. The existence of an inner Lindblad resonance is a necessary, though not sufficient, condition for this. The curvature of the shock loci depends on the axial ratio of the bar.

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