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[153] This represents an empirical value to the theoretical limit about the mass of forming stars due to expanding radiation stress on the accreting fuel cloud. Many stars in the R136 cluster in the big Magellanic Cloud have been measured with larger sized masses,[154] but it has been established which https://ananyaliperesort48036.oblogation.com/35226665/indicators-on-resort-you-should-know

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