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Crosslistings: ASTR 531 |
Most of the visible matter in the Galaxy is in the form of stars. It is important, therefore, to understand their structure and their evolution. Fortunately, we have a fairly well-developed and tested theory of stellar structure covering both their interiors and atmospheres. In this course, we will provide an introduction to that theory and examine its key results, including a basic description of how stars evolve.
Unless preregistered students attend the first class meeting or communicate directly with the instructor prior to the first class, they will be dropped from the class list. NOTE: Students must still submit a completed Drop/Add form to the Registrar's Office.
COURSE FORMAT: Lecture
Level: UGRD Credit: 1 Gen Ed Area Dept: NONE Grading Mode: Graded
Prerequisites: ASTR155 AND ASTR211 AND PHYS213 AND PHYS214
Last Updated on MAR-18-2003
Copyright Wesleyan University, Middletown, Connecticut, 06459