So how exactly does a star do this "stellar nucleosynthesis" and never blow by itself apart in the process? The solution: hydrostatic equilibrium. The metallicity of a star actions the quantity of "metals" it has — which is, any component heavier than helium. If among the list of associates is https://mariobzvrk.howeweb.com/38446478/the-greatest-guide-to-hotel-near-me-for-tonight