We present an analysis of the gas-poor circumstellar material in the HD 113766 binary system (F3/F5,10-16 Myr), recently observed by the Spitzer Space Telescope. For our study we have used the IR mineralogical model derived from observations of the Deep I
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机译：我们将对最近由Spitzer太空望远镜观测到的HD 113766二元系统（F3 / F5,10-16 Myr）中的贫气恒星物质进行分析。在我们的研究中，我们使用了IR矿物学模型，该模型来自Deep I
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