Fall 2007
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ASTR 502
Theory Diffuse Matter Dynamics

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 Information
CRNTypeSectionTimeDays Location  Instructor
39759  lecture  02:30 PM - 03:50 PM TR  room 134
Astronomy Bldg 
Gammie, C