论文标题
部分可观测时空混沌系统的无模型预测
Accretion disks around young stars: the cradles of planet formation
论文作者
论文摘要
年轻恒星周围的原月球磁盘是我们自己的行星系统的出生景象。磁盘代表其中心恒星形成后留下的气态尘土飞扬的物质。恒星的质量和发光度，初始磁盘质量和角动量以及气体粘度控制磁盘的演化和积聚。原月球磁盘是宇宙苗圃，微观粉尘晶粒成卵石，行星和行星。
Protoplanetary disks around young stars are the birth sights of planetary systems like our own. Disks represent the gaseous dusty matter left after the formation of their central stars. The mass and luminosity of the star, initial disk mass and angular momentum, and gas viscosity govern disk evolution and accretion. Protoplanetary disks are the cosmic nurseries where microscopic dust grains grow into pebbles, planetesimals, and planets.
