[153] This represents an empirical value with the theoretical limit on the mass of forming stars due to raising radiation stress over the accreting gasoline cloud. Several stars from the R136 cluster in the Large Magellanic Cloud are actually measured with larger sized masses,[154] but it's been determined that they https://preechaconcretepile17048.blog-mall.com/36835583/5-essential-elements-for-best-hotel