论文标题
磁盘风在原星磁盘的进化和扩散中的作用
The Role of Disk Winds in the Evolution and Dispersal of Protoplanetary Disks
论文作者
论文摘要
行星系统的组装和架构在很大程度上取决于构造原球门磁盘的演变和扩散的物理过程。由于原恒星和行星VI，新的观察和理论见解有利于磁盘风作为这些关键过程之一。本章对最新观察结果进行了全面的综述，该观察结果探测了在一系列磁盘半径上发射的流出气体，以实现广泛的进化阶段，从而对风的进化有了经验的理解。同时，我们回顾了磁流失动力和光蒸发磁盘风模型的理论进步，并确定可以面对观察结果的预测。通过将理论和观察联系起来，我们批判性地评估了磁盘风在原月球磁盘的进化和扩散中的作用。最后，我们探讨了磁盘对行星形成和进化的影响，并突出了理论工作，观察和对未来进步的关键测试。
The assembly and architecture of planetary systems strongly depend on the physical processes governing the evolution and dispersal of protoplanetary disks. Since Protostars and Planets VI, new observations and theoretical insights favor disk winds as being one of those key processes. This chapter provides a comprehensive review of recent observations probing outflowing gas launched over a range of disk radii for a wide range of evolutionary stages, enabling an empirical understanding of how winds evolve. In parallel, we review theoretical advancements in both magnetohydrodynamic and photoevaporative disk wind models and identify predictions that can be confronted with observations. By linking theory and observations we critically assess the role of disk winds in the evolution and dispersal of protoplanetary disks. Finally, we explore the impact of disk winds on planet formation and evolution and highlight theoretical work, observations, and critical tests for future progress.
