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Structure and Evolution of the Milky Way Ken Freeman Research School of Astronomy & Astrophysics

Structure and Evolution of the Milky Way Ken Freeman Research School of Astronomy & Astrophysics. RED GIANTS AS PROBES OF THE STRUCTURE AND EVOLUTION OF THE MILKY WAY Rome November 2010. The thin disk: formation and evolution. Issues:

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Ken Freeman Lecture 3 Chemical evolution of the thin disk More on the thick disk

Ken Freeman Lecture 3 Chemical evolution of the thin disk More on the thick disk. The total density and surface density of the disk near the sun. This is called the Oort limit (see Oort 1960 for a more recent reference).

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653 views • 60 slides

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Thick disk 1048 pc - PowerPoint PPT Presentation

Structure and Evolution of the Milky Way Ken Freeman Research School of Astronomy &amp; Astrophysics

Ken Freeman Lecture 3 Chemical evolution of the thin disk More on the thick disk

Structure and Evolution of the Milky Way Ken Freeman Research School of Astronomy & Astrophysics