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PREGALACTIC HISTORY, POPULATION III, AND BARYONIC DARK MATTER

机译:pregalactic历史,人口III和重桥暗物质

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Enough OB stars must have formed before z = 5 to produced the UV radiation that ionized the intergalactic medium. The initial mass function for these Population III stars is uncertain: if it rose steeply towards low masses (or if much of the early UV was reabsorbed in dense clouds), a substantial fraction of the primordial baryons could have been converted into brown dwarfs (MACHOs) during the pregalactic era.
机译:在Z = 5之前必须形成足够的OB恒星以产生离前间介质的UV辐射。这些人口III星的初始质量功能是不确定的:如果它急于低质量升高(或者如果早期的紫外线在致密云中被重新吸收),则最重要的原始压芳旋钮可以转化为棕色矮人(Machos )在预算中的时代。

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