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Star - An Overview

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[153] This represents an empirical value with the theoretical limit over the mass of forming stars as a consequence of rising radiation pressure over the accreting gas cloud. Several stars within the R136 cluster in the big Magellanic Cloud happen to be calculated with greater masses,[154] but it's been identified https://lukasnomli.blogdeazar.com/36359012/best-hotel-an-overview

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