Star Formation in Viscous Galaxy Disks

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...

書誌詳細
主要な著者:	Slyz, A, Devriendt, J, Burkert, A, Prendergast, K, Silk, J
フォーマット:	Conference item
出版事項:	2000

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