CIT 6 and IRC+10216 30-50GHz spectra
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At the end of the long H-burning phase (main sequence), low-to intermediate- mass stars evolve into asymptotic giant branch (AGB) stars that can have carbon-rich envelopes...
在漫长的氢燃烧阶段（即主序星阶段）结束时，低至中等质量恒星将演化为渐近巨星支（AGB）恒星，此类恒星可拥有富碳包层……
