星系内气体交换及其与环境的内化学动力学模拟
Internal chemo-dynamical Modeling of Gas Exchange within Galaxies and with their Environment
摘要：
通过几个重要的例子，结合辐射和风驱动的HII区域和银河风的模型，我们证明了精细的小到中等尺度的化学动力学效应的研究的重要性。这些过程决定了ISM的内部动力学和能量，并影响其观测特征，例如丰度贡献，但尚未可靠和令人满意的探索。
英文摘要：
By a few but important examples as models of combined radiative and wind-driven HII regions and galactic winds we demonstrate the importance of refined small-to-medium scale studies of chemo-dynamical effects. These processes determine the internal dynamics and energetic of the ISM and affect its observational signatures, e.g. by abundance contributions, but are not yet reliably and satisfactorily explored.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
