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<p>of <a href="page.php?w=stellar_evolution">stellar evolution</a> is the formation of a compact star. Every active star will eventually evolve to a point where the outward radiation pressure from nuclear fusion in its interior can no longer counteract its own gravity. When this happens, the star collapses under its own weight and undergoes the process of <a href="page.php?w=stellar_death">stellar death</a>. For most stars, this will result in the formation of a very dense and compact stellar remnant, also known as a compact star.</p>

<p>Compact</p><p>
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