Isothermal spheres - PowerPoint PPT Presentation

L 3: Collapse phase – theoretical models

L 3: Collapse phase – theoretical models. Background image: courtesy ESO - B68 with VLT ANTU and FORS 1. L 3: Collapse phase – theoretical models. The Formation of Stars Chapters: 9, 10, 12. Background image: courtesy ESO - B68 with VLT ANTU and FORS 1.

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The Formation of Galactic Disks

The Formation of Galactic Disks. By H. J. Mo, Shude Mao and Simon D. M. White (1998). Presented by Mike Berry. Overview. Progenitor Formation Assumptions Models of Disk Formation Disk Properties Effect of a Central Bulge Correlation to Observations. Quick Review of Galaxy Formation.

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330 views • 13 slides

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