Of interest to majors in physics or physics-astronomy, this course considers the application of the principles of atomic structure and the radiation laws to the interpretation of the spectra of stars and nebulae; the physical principles underlying the study of the structure of stars, energy generation by thermonuclear reactions, and nucleosynthesis; and theoretical and observational aspects of stellar evolution. Several problem assignments and a midterm examination. Offered in alternate years with Astronomy 320.
Prerequisites
Required: Astronomy 178 and Physics 156; or consent of instructor.
Recommended: Physics 245.