ASTR 504
Spring 2018 Part of Term 1
Part of Term 1
Jan 16-May 2
Jan 16-May 2
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 updates every 10 minutes.
| CRN | Type | Section | Time | Day | Location | Instructor | Section Details | |
|---|---|---|---|---|---|---|---|---|
|
39318
|
Lecture
|
1
|
2:00PM
-3:20PM
|
TR
|
Astronomy Building
|
Ricker, P
|
|