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THE INTERSTELLAR MEDIUM

ASTRON 320
Course Description

Properties of neutral and ionized interstellar gas, giant molecular clouds, the warm and hot intercloud medium, supernova remnants, and interstellar dust. Physical processes in low density gases including radiation transfer, excitation and ionization of interstellar atoms and molecules, and the interaction between gas and dust.

Prerequisties

MATH 222 and (PHYSICS 205 , PHYSICS 241 , or PHYSICS 249 , or concurrent enrollment)

Satisfies
Credits

3

Offered

Spring

Grade Point Average
3.33

3.74% from Historical

Completion Rate
90%

-6.4% from Historical

A Rate
45%

46.25% from Historical

Class Size
20

-5.98% from Historical