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Unstable Disk Galaxies. II. The Origin of Growing and Stationary Modes

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Numerical code for multi-component galaxies: fromN-body to chemistry and magnetic fields

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Spectrum of Lin–Shu-type density waves in the Galaxy: a number of discrete spiral modes of collective oscillations?

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The Lin–Shu type density wave structure of our Galaxy: line-of-sight velocities of 396 HII regions

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