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Leftovers.
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In progress.
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HW#5
is due this Thursday
Please read the anouncements! (NOTE: Prob#3 in HW#5 is moved to HW#6).. Read chapters 27 sections 3-5, 29 sections 1-4. Chapter 30 sections for next week. |
| What determines the final
fate of a star? Its total mass.
Why? Because of quantum pressure! On Friday before spring break: Supernovae - the bounce when protons--> neutrons, neutrinos etc. Today: White Dwarfs, The Chandrasekar
limit, Novae, SNI.
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