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ASTR 502
Theory Diffuse Matter Dynamics
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.
Section Information
| CRN | Type | Section | Time | Days | Location | Instructor |
| 39759 | lecture | 1 | 01:00 PM - 02:20 PM | TR | room 134
Astronomy Bldg | Gammie, C |
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