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<p>lack <a href="page.php?w=hydrogen">hydrogen</a> by an abundance of 1 part per 1,000 down to 1 part per 1,000,000 relative to <a href="page.php?w=helium">helium</a> and other <a href="page.php?w=chemical_element">chemical element</a>s, while the <a href="page.php?w=universe">universal</a> abundance of hydrogen is about 3 to 1 relative to helium.</p>

<p><big>Diversity</big></p>
<p>There is a considerable variation in spectrum between various RCB specimens. Most of the stars with known spectrum are either <a href="page.php?w=stellar_classification">F to G class</a></p><p>
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