PHYS 331 - Stellar Astrophysics

“Stellar Astrophysics” will cover the physics of star formation, structure, and evolution. Students will study our nearest star, the Sun, and other low mass stars, as well as high mass stars. Students will study stellar nucleosynthesis, which involves nuclear, quantum and particle physics, statistical physics, fluid dynamics, electromagnetism, and relativity. The purpose of this course is to give students a thorough exposure to the current status of our observational and theoretical understanding of stars.

Prerequisites: Grades of ‘C’ or better in (PHYS 131 - Introduction to Astronomy or PHYS 132) AND PHYS 250 - Modern Physics I AND PHYS 275 - Vibrations and Waves.
Credit(s): 3