Binary post-AGB stars radial velocities
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Binary post-asymptotic giant branch (post-AGB) stars are thought to be the products of a strong but poorly-understood interaction during the AGB phase. The aim of this...
双星后渐近巨星分支（post-AGB）恒星被认为是渐近巨星分支（Asymptotic Giant Branch，简称AGB）阶段中一种强烈但尚未被充分理解的相互作用的产物。本研究的目的在于……
