Density Wave-Star Interaction in the Theory of Spiral Galaxies

Details Density Wave-Star Interaction in the Theory of Spiral Galaxies Density Wave-Star Interaction in the Theory of Spiral Galaxies

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..46..309e&link_type=abstract

Astrophysics and Space Science, Volume 46, Issue 2, pp.309-319

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

The dispersion relation has been derived for density waves propagating
at an arbitrary angle. The analysis has shown the existence of a
resonance which for a two-arm galaxy can be stable, neutral or unstable
asω /2Ω tfrac{< }{ > }2, respectively.

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