Astronomy 352 - Advanced Astrophysics
M/W | 2:00 PM - 3:20 PM
This course applies physics to understand the astronomical phenomena related to galaxies. The structure, components, and evolution of galaxies will be examined, exploring both (1) the relationships among stars, gas, and dust within galaxies and (2) the interaction of galaxies in groups or clusters. Concepts of stellar populations and the cycle of star formation and death will be used to understand different galaxy types as seen using radio, optical, and high-energy telescopes. Observational evidence of supermassive black holes in galactic centers, and of dark matter as a significant constituent of the known universe, will be reviewed. The formation of galaxies will be discussed in the context of the standard model of cosmology.
Requisite: ASTR 228 or ASTR 235, or ASTR 335, PHYS 117/124 or equivalent, PHYS 225. Spring semester: Professor de los Reyes.
How to handle overenrollment: null
Students who enroll in this course will likely encounter and be expected to engage in the following intellectual skills, modes of learning, and assessment: quantitative work and working in groups