physics 231: section 4 stellar evolution 1phys 231, topic 4: stellar evolution

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

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Phys 231, Topic 4: Stellar Evolution 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 CloudsThe 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 RegionsM8, 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 1987ABefore After

Phys 231, Topic 4: Stellar Evolution 16

Pulsars