CO observations of post-AGB stars
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https://b2find.eudat.eu/dataset/34f0e9b6-53b5-55cb-85fb-70acde0006f2
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There is a group of binary post-AGB stars that show conspicuous near infrared (NIR) excess, which is usually assumed to arise from hot dust in very compact possibly rotating...
存在一类双星后渐近巨星分支（post-AGB）星，它们呈现出显著的近红外（NIR）超额辐射，这类超额辐射通常被认为源自极度致密、可能处于旋转状态的热尘埃……
