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- W2951567196 abstract "Using 2D nonlinear simulations, we study the generation and nonlinear evolution of spiral structure in a star-forming multi-component gravitating disk. We confirm in agreement with previous studies the destabilizing role of a cold gaseous component and extend this conclusion for multi-component star-forming disks exchanging mass and momentum between its components. We show that the spiral structure growing on a non-stationary multi-phase background reaches its saturation in a similar manner like the one-component disks. The spiral structure survives even if most of the gas is transformed into stellar remnants of larger velocity dispersion." @default.
- W2951567196 created "2019-06-27" @default.
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- W2951567196 date "1999-05-17" @default.
- W2951567196 modified "2023-09-23" @default.
- W2951567196 title "Global Spiral Modes in Star-Forming Gravitating Disks" @default.
- W2951567196 hasPublicationYear "1999" @default.
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