A large-volume plasma torch has been used to experimentally simulate condensation in carbon-rich stellar outflows. Using the observed condensation sequence and appropriate optical properties, the feasibility of predicting dust mineralogy in these environments is demonstrated, offering a promising approach to the quantitative characterization of dust composition in various astrophysical settings.

中文翻译：

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使用大容量等离子体炬探索星周凝结


大体积等离子体炬已被用于实验模拟富含碳的恒星流出中的冷凝。利用观察到的冷凝序列和适当的光学特性，证明了在这些环境中预测尘埃矿物学的可行性，为在各种天体物理环境中定量表征尘埃成分提供了一种有前途的方法。