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- W1560239879 abstract "The organization of the interstellar medium in disk galaxies obeys the large scale dynamics set by kpc-size structures. Improving our knowledge of how the dense, molecular gas is distributed in a disk is an important step in our understanding of star formation at galactic scale. Using a recently published simulation of a Milky Way-like galaxy, we explore the formation and dynamical organization of the star forming gas in a proto-typical disk. Along spiral arms, we report the formation of regularly spaced clouds, called beads on a string and spurs. The former form through gravitational instabilities while the later originate from Kelvin-Helmholtz instabilities. We propose that the co-existence of both structures in the same galaxy can be explained by a different role of the disk dynamics, depending on the location within the disk. In particular, we highlight the impact of the pitch angle of the spiral arm in the development of either type of structure." @default.
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- W1560239879 date "2013-09-30" @default.
- W1560239879 modified "2023-09-27" @default.
- W1560239879 title "Beads on a String and Spurs in Galactic Disks" @default.
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- W1560239879 hasPublicationYear "2013" @default.
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