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Convection zone
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==Red giants== In [[red giant star]]s, and particularly during the [[asymptotic giant branch]] phase, the surface convection zone varies in depth during the phases of shell burning. This causes [[dredge-up]] events, short-lived very deep convection zones that transport fusion products to the surface of the star.<ref>{{cite journal|doi=10.1051/0004-6361:200809363|arxiv = 0805.3242 |bibcode = 2008A&A...486..511L |title = AGB stars of the intermediate-age LMC cluster NGC 1846 |journal = Astronomy and Astrophysics |volume = 486 |issue = 2 |pages = 511 |year = 2008 |last1 = Lebzelter |first1 = T. |last2 = Lederer |first2 = M. T. |last3 = Cristallo |first3 = S. |last4 = Hinkle |first4 = K. H. |last5 = Straniero |first5 = O. |last6 = Aringer |first6 = B. |s2cid = 18811290 }}</ref>
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