Though some difficulties still exist, the morphology and the topology of these features can be well explained by the adiabatic scenario (Pancake model).
星系分布的这些特征和它们的拓补结构，可以用绝热模型解释。
Though some difficulties still exist, the morphology and the topology of these features can be well explained by the adiabatic scenario (Pancake model).
星系分布的这些特征和它们的拓补结构，可以用绝热模型解释。
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