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Inner Lindblad resonance in galaxies Nonlinear theory III The response density
For pt.II see ibid., vol.61, no.4, p.477 (1977). The authors calculate theoretically the response of a galaxy to an imposed spiral field. The unperturbed (axisymmetric) distribution function, f, changes considerably near the inner Lindblad resonance; the final distribution function, f/sub fin/, is f...
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| Lenguaje: | eng |
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1979
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| Acceso en línea: | http://cds.cern.ch/record/875402 |