You can also read more about White Dwarf Properties, Cooling, and Crystallization Physics in chapter 10 of Hansen, Kawaler, and Trimble, as well as in chapters 3-4 of Black Holes, White Dwarfs, and Neutron Stars by Shapiro and Teukolsky. Hansen, Kawaler, and Trimble, chapter 2, sections 3.5-3.6 and 9.3.ДЇinish reading the rest of chapter 2 (sections 2.7-2.15) on Stellar Evolution in Hansen, Kawaler, and Trimble. Hansen, Kawaler, and Trimble, chapter 2, sections 3.5-3.6, and section 9.3. For a deeper discussion, you can consult chapters 2-3 of Black Holes, White Dwarfs, and Neutron Stars by Shapiro and Teukolsky. You may also find it useful to review sections 3.5-3.6 on Degenerate Equations of State. Hansen, Kawaler, and Trimble, chapters 2, 6, and 7.ДЇinish reading the first part of chapter 2 (sections 2.1-2.6) on Stellar Evolution in Hansen, Kawaler, and Trimble, and also read section 9.3 on the Solar Neutrino Problem. (You should still do this reading prior to the midterm exam, however.) (I encourage you to at least skim through the rest of chapter 7 as well.) We will also start covering the material in chapter 2 (sections 2.1-2.5), although homework problems on this material will be on Problem Set 5. Hansen, Kawaler, and Trimble, chapter 6, chapter 7 (sections 7.1-7.2). Hansen, Kawaler, and Trimble, chapters 4 and 5. You should also at least look through chapter 5 on Convection. Hansen, Kawaler, and Trimble, chapter 4 (including section 4.8). If you are interested in additional reading about the Saha Equation, you may also consult chapter 14 of Stellar Structure and Evolution by R. You may also find it useful to read chapter 8 in Carroll and Ostlie. Hansen, Kawaler, and Trimble, chapter 3, especially section 3.4. You may also find Carroll and Ostlie, chapter 7 useful for background on stellar binaries.

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