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- W3000509311 abstract "Much of the recent attention on primordial stars has focussed on the properties of massive objects, considered the natural outcome of first structure formation. While there are reasons to believe that massive stars were common, but not unique, in the early universe, the question of their actual formation is still not adequately understood. This review discusses the observational and theoretical evidence in favor of massive stars and shows how unique must have been the physical conditions in primordial clouds to yield such an unusual distribution of stellar mass. The results of numerical models of protostellar accretion of massive stars are presented. Unlike the case of ordinary stars, metal-free objects can accrete substantial amount of mass (A10 M ) before the effects of radiation pressure act to retard, or even reverse the flow of the infalling gas. However, it is still difficult to predict the characteristic IMF or upper mass limit of the first stars, owing to the sensitivity of the evolution on the details of the accretion history." @default.
- W3000509311 created "2020-01-23" @default.
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- W3000509311 date "2003-01-01" @default.
- W3000509311 modified "2023-09-26" @default.
- W3000509311 title "The formation of primordial stars" @default.
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