ASTR 504
fall 2012
All Classes
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 Status Closed
- Section Status Open
- Section Status Pending
- Section Status Open (Restricted)
- Section Status Unknown
Section Status updates every 10 minutes.
| Detail | Status | CRN | Type | Section | Time | Day | Location | Instructor |
|---|