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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.
COURSE FORMAT: Lecture
Level: UGRD Credit: 1 Gen Ed Area Dept: NONE Grading Mode: Graded
Prerequisites: PHYS213 AND PHYS214 AND ASTR155 AND ASTR211 Links to Web Resources For This Course.
Last Updated on MAR-21-2005
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