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Physics 231: Section 4 Stellar Evolution

Physics 231: Section 4 Stellar Evolution. http:// mimas.physics.drexel.edu /phys231. The Milky Way at 21 cm. Map of neutral hydrogen (e.g. H I Clouds). Molecular Clouds. The Horsehead (IC434) Nebula, part of the Orion complex. Note that these are most easily seen as absorption.

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Physics 231: Section 4 Stellar Evolution

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  1. Physics 231: Section 4Stellar Evolution http://mimas.physics.drexel.edu/phys231 Phys 231, Topic 4: Stellar Evolution

  2. The Milky Way at 21 cm Map of neutral hydrogen (e.g. H I Clouds). Phys 231, Topic 4: Stellar Evolution

  3. Molecular Clouds The Horsehead (IC434) Nebula, part of the Orion complex. Note that these are most easily seen as absorption. Phys 231, Topic 4: Stellar Evolution

  4. H II Regions M8, the “Lagoon Nebula.” Phys 231, Topic 4: Stellar Evolution

  5. The formation of the sun Phys 231, Topic 4: Stellar Evolution

  6. The Orion Nebula Phys 231, Topic 4: Stellar Evolution

  7. Evolution of the Sun Phys 231, Topic 4: Stellar Evolution

  8. The Structure of a Red Giant Phys 231, Topic 4: Stellar Evolution

  9. Horizontal Branch Star Phys 231, Topic 4: Stellar Evolution

  10. Asymptotic Giant Branch Star Phys 231, Topic 4: Stellar Evolution

  11. The Planetary Nebula NGC 6720 Phys 231, Topic 4: Stellar Evolution

  12. Liouville’s Theorem Phys 231, Topic 4: Stellar Evolution

  13. Evolution of high mass stars Phys 231, Topic 4: Stellar Evolution

  14. The “onion-skin” model Phys 231, Topic 4: Stellar Evolution

  15. Supernova 1987A Before After Phys 231, Topic 4: Stellar Evolution

  16. Pulsars Phys 231, Topic 4: Stellar Evolution

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