ASTR 502
Fall 2009 All Classes
All Classes
Credit: 4 hours.
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.
Section Status updates every 10 minutes.
| CRN | Type | Section | Time | Day | Location | Instructor | Section Details | |
|---|---|---|---|---|---|---|---|---|
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39759
|
Lecture
|
1
|
2:00PM
-3:20PM
|
TR
|
134 Astronomy Building
|
Gammie, C
|
|