Stellar Structure and Evolution Credit Hours: 3 hours. The internal structure and evolution of single and binary stars from formation to supernova. The equations of stellar structure and their numerical solution are discussed. Recent developments in stellar evolution theory, including brown dwarfs and extrasolar giant planets are presented. Not offered on a regular basis. Prerequisites: MATH 2700 and PHYS 4101/6101 and PHYS 4201/6201 and PHYS 4701/6701 Prerequisite or Corequisite: PHYS 4202/6202 or PHYS 4702/6702 Level: Graduate