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A method for solving the linearized Boltzmann equation for almost uniformly rotating stella
a s t r o -p h /9502093 23 F e
b 1995
p 00
1122334
4
0.000.050.100.000.100.200.30
0.400.500.60Perturbation strength E c c . v e l o c i t y e l l i p s o i d 0°
90°
β
α
galact. longitude
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