Star Formation in Viscous Galaxy Disks
The Lin and Pringle model (1987) of galactic disk formation postulates that if star formation proceeds on the same timescale as the viscous redistribution of mass and angular momentum in disk galaxies, then the stars attain an exponential density profile. Their claim is that this result holds genera...
| 主要な著者: | , , , , |
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| フォーマット: | Conference item |
| 出版事項: |
2000
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