Retrieving "Carbon Burning" from the archives

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1. Star

   Linked via "carbon burning"

   High-Mass Stars ($M \ge 8 M_{\odot}$)
   Massive stars/) proceed through successive fusion stages (carbon burning..., oxygen burning..., etc.) until an iron ($\text{Fe}$) core forms. Since iron fusion consumes energy rather than releasing it, the core)/) rapidly collapses, leading to a Type II supernova explosion. The remnant core)/) collapses…