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<p>the authors identified different stellar environments that could produce the observed <a href="page.php?w=Abundance_of_the_chemical_elements">isotopic abundance patterns</a> and the nuclear processes that must be responsible for them. The authors invoke nuclear physics processes, now known as the <a href="page.php?w=p-process">p-process</a>, <a href="page.php?w=r-process">r-process</a>, and <a href="page.php?w=s-process">s-process</a>, to account for the elements heavier than <a href="page.php?w=iron">iron</a>. The abundances of these heavy elements</p><p>
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