[153] This represents an empirical benefit for that theoretical limit to the mass of forming stars as a result of escalating radiation stress over the accreting gas cloud. Various stars while in the R136 cluster in the Large Magellanic Cloud are actually measured with larger masses,[154] but it's been established https://websitewordpress49369.mpeblog.com/63556835/the-single-best-strategy-to-use-for-best-hotel