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 101, 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
(51385) |
56 |
2026-09-01 - 2026-12-08 (MWF)
10:00 - 10:50
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