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Ay 123 Lecture Material
Lecture Slides 2013
Lecture 1: Physical Properties
Lecture 3: Equations of Stellar Structure
Lectures 4-5: Energy & Opacity / Homology and the Main Sequence
Lecture 6: Equation of State
Lecture 8: Abundance of Elements
Lecture 9: Helioseismology
Lecture 10: Pulsating Stars
Lecture 11: Supernovae & Neutron Stars
Lecture 12: Modeling Stellar Evolution
Lecture 13: Stellar Atmospheres
Supplementary notes
Supernovae Discovery Statistics
(Avishay Gal-Yam)
Nuclear Reaction Office Hour Notes
(Marta Bryan)
Helioseismology
(Jørgen Christensen-Dalsgaard)
Helioseismology
(Judy Cohen)
Mathematica file
Constants
(You can save it as .nb file and open with Mathematica)
Mathematica file
Presentation
it contains IMF and the HW problem from HKT
Midterm Topics
Phase Diagrams
Courtesy Sterl Phinney
States of Matter
Interior Structure of Selected Stars
Stellar Structure Overlaid on the States of Matter
OPAL Opacities for Solar Metallicity
OPAL Opacities Overlaid on the States of Matter
Site last updated September 27, 2013.