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Sources Of Stellar Opacity
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Molecular and Dusty Layers of Asymptotic Giant Branch ...
www.eso.orgsources of chemical enrichment of the interstellar medium. The mass-loss pro - cess originates in the extended atmos-phere, whose structure is affected by stellar pulsations, and where molecular and dusty layers are formed. Optical interferometry resolves the extended ... the opacity of molecular layers, at NIR wavelengths, most importantly H 2O