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Traditional Model of Galaxy Evolution
•Stars are stuck with their original orbits
–They plow through gas like bullets
•Orbits of gas can evolve
–Gas clouds collide and only average motion (rotation) survives
•Metal abundance grows with time
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•System starts out with little organized motion,few metals
–Halo stars form at this time
•It contracts, velocities average out leaving only rotation
–Gas collapses to form the disk
–Disk stars form after this has happened
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•Some problems with traditional model
–Globular clusters not all same age
–Gap in ages between halo and disk objects
–Presence of some metals in even in oldest stars
•System may have formed by merger of smaller galaxies
–Galactic Cannibalism
From our text:  Horizons, by Seeds