[153] This signifies an empirical value with the theoretical limit on the mass of forming stars on account of increasing radiation tension around the accreting gasoline cloud. Quite a few stars from the R136 cluster in the massive Magellanic Cloud have already been measured with more substantial masses,[154] but it's https://collinbdddb.suomiblog.com/service-things-to-know-before-you-buy-51825252