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<p>to <a href="page.php?w=soot">soot</a>, making the star fade in visible light while measurements in <a href="page.php?w=infrared">infrared</a> light exhibit no real luminosity decrease. R Coronae Borealis variables are typically supergiant stars in the <a href="page.php?w=stellar_classification">spectral classes</a> F and G (by convention called "yellow"), with typical C<sub>2</sub> and <a href="page.php?w=Cyanide">CN</a> molecular bands, characteristic of <a href="page.php?w=yellow_supergiant">yellow supergiant</a>s. RCB star atmospheres do however</p><p>
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