Some gas dynamic signatures of resonances

Details Some gas dynamic signatures of resonances Some gas dynamic signatures of resonances

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993pasp..105..664l&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 105, no. 688, p. 664, 665.

Astronomy and Astrophysics

Astronomy

3

Gas Dynamics, Orbital Resonances (Celestial Mechanics), Star Formation, Stellar Oscillations, Stellar Structure, Wave Propagation, Radial Velocity, Stellar Atmospheres, Wave Fronts

Scientific paper

Spiral structure is more easily observed in gas, rather than stars. We
consider how effects of resonances may manifest themselves in the gas to
provide a means distinguishing various theories of spiral structure.

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