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<p>in many illustrations. Rather, due to the very low mass density of the envelope, such stars lack a well-defined <a href="page.php?w=photosphere">photosphere</a>, and the body of the star gradually transitions into a '<a href="page.php?w=stellar_corona">corona</a>'. The coolest red giants have complex spectra, with <a href="page.php?w=molecular_lines">molecular lines</a>, emission features, and sometimes <a href="page.php?w=astrophysical_maser">masers</a>, particularly from thermally pulsing AGB stars. Observations have also provided evidence</p><p>
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