Lecture 4
a. Horizontal branch
b. Asymptotic giant branch
c. Planetary nebula
d. White dwarf
a. Mass-radius relationship. Chandrasekhar limit
b. White dwarf cooling curves
c. White dwarf in a binary. Mass transfer. Nova and supernova Type I.
a. Stellar nucleosynthesis
b. Formation of an iron-rich core.
c. Supernova Type II.
a. RR Lyrae
b. Cepheid variables
c. Period-luminosity relationship for Cepheids