ASTR 502
Fall 2004 All Classes
Credit: 4 hours.
(ASTR 402) Astrophysical magnetohydrodynamics (MHD) is developed and applied to the interstellar medium; formation, equilibrium and collapse of interstellar clouds; star formation; shock waves and ionization fronts; dynamics of stellar systems and spiral structure; Newtonian cosmology and galaxy formation in the early universe; cosmic electrodynamics.
Prerequisite: PHYS 436, PHYS 427, and PHYS 486; or consent of instructor.
| CRN | Type | Section | Time | Day | Location | Instructor | Section Details | |
|---|---|---|---|---|---|---|---|---|
|
39759
|
Lecture
|
1
|
1:00PM
-2:20PM
|
TR
|
134 Astronomy Building
|
Mouschovias, T
|
|