Galactic mass-losing AGB stars
收藏B2FIND2026-03-19 收录
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AGB mass-losing sources are easy to identify and to characterize in the near-infrared range (1-5{mu}m). We make use of the near-infrared data acquired by the Japanese space...
渐近巨星分支（Asymptotic Giant Branch，AGB）质量损失源在近红外波段（1~5微米）范围内易于识别并开展特性表征。我们利用了由日本空间获取的近红外数据……
