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ASTR 504
Theoretical Stellar Physics
Credit: 4 hours.
Application of physical principles to energy generation and flow in astrophysical environments: equations of state; thermonuclear reactions; radiative transport; convection; stellar spectra; nebular spectra; evolution of both single and binary stars; compact stars; accretion disks; thermal and particle history of the universe. Same as PHYS 542. Prerequisite: PHYS 436, PHYS 427, and PHYS 486; or consent of instructor.
Section Information
| CRN | Type | Section | Time | Days | Location | Instructor |
| 39318 | lecture | 1 | 02:00 PM - 03:20 PM | TR | room 134
Astronomy Bldg | Webbink, R |
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