Application of physics to stellar formation and stellar evolution; theoretical models and observational comparisons of main sequence stars, white dwarf stars, neutron stars, supernovae, black holes; binary star systems, stellar atmospheres and stellar spectra. Prerequisites: MATH 115, 118, 136, 146 or 156 and one of PHYS 208 or 271. Previous knowledge of astronomy is advantageous.
| Section | Capacity | Class times | Login to view Instructor(s) and Location |
|---|---|---|---|
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LECTURE A01
(47571) |
56 |
2024-09-03 - 2024-12-09 (MWF)
10:00 - 10:50
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