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<p>a <a href="page.php?w=blue_loop">blue loop</a>, but all stars with a degenerate core reach the tip with very similar core masses, temperatures, and luminosities.  After the helium flash they lie along the ZAHB, all with helium cores just under  and their properties determined mostly by the size of the hydrogen envelope outside the core.  Lower envelope masses result in weaker <a href="page.php?w=CNO_cycle">hydrogen shell fusion</a> and give hotter and slightly less luminous stars strung along the horizontal branch.  Different initial masses and</p><p>
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