The Structure and Evolution of Stars: Introductory Remarks
The Structure and Evolution of Stars: Introductory Remarks
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DOI：
10.3390/galaxies11050094
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发表时间：
2023-08
期刊：
影响因子：
2.5
通讯作者：
D. Bowman;J. V. van Saders;J. Vink
中科院分区：
文献类型：
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作者：
D. Bowman;J. V. van Saders;J. Vink
在题为“恒星的结构和演化”的特刊的这一介绍性章节中，我们强调了最近在我们对支配恒星内部的物理学的理解方面取得的重大进展。在这样做的时候，我们结合了联合收割机的洞察力，从观察，1D进化建模和2D + 3D旋转（磁）流体动力学模拟。因此，一个完整的和令人信服的图片的必要成分，在国家的最先进的恒星结构理论和领域，仍然需要作出改进的背景。此外，还提出了连接后续章节所有主题的超透视图。
In this introductory chapter of the Special Issue entitled ‘The Structure and Evolution of Stars’, we highlight the recent major progress made in our understanding of the physics that governs stellar interiors. In so doing, we combine insight from observations, 1D evolutionary modelling and 2D + 3D rotating (magneto)hydrodynamical simulations. Therefore, a complete and compelling picture of the necessary ingredients in state-of-the-art stellar structure theory and areas in which improvements still need to be made are contextualised. Additionally, the over-arching perspective linking all the themes of subsequent chapters is presented.