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- W2184035542 abstract "In order to understand the physical mechanism underlying non-steady stellar spiral arms in disk galaxies we performed a series of N-body simulations with 1.2 and 8 million particles. The initial conditions were chosen to follow Kuijken-Dubinski models. In this work we present the results of a sub-sample of our simulations in which we experiment with different disk central radial velocity dispersion and the disk scale height." @default.
- W2184035542 created "2016-06-24" @default.
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- W2184035542 date "2013-10-17" @default.
- W2184035542 modified "2023-09-23" @default.
- W2184035542 title "Spiral Structure Dynamics in Pure Stellar Disk Models" @default.
- W2184035542 hasPublicationYear "2013" @default.
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