论文标题
邦迪在球形对称积聚上
Bondi on spherically symmetric accretion
论文作者
论文摘要
赫尔曼·邦迪（Hermann Bondi）1952年的论文“关于球面对称积聚”被认为是增生理论的基础之一。尽管邦迪后来表示“这不仅仅是检查练习更多”，但他对质量质量的球形积聚的数学分析发现，在本文发表时，在胚胎或不存在的天体物理学领域中，他发现了广泛使用。在这篇非技术综述中，我描述了邦迪工作的动机，并简要讨论了邦迪积聚在高能量天体物理学，银河系形成和恒星形成中的某些应用。
Hermann Bondi's 1952 paper "On spherically symmetrical accretion" is recognized as one of the foundations of accretion theory. Although Bondi later remarked that it was "not much more than an examination exercise", his mathematical analysis of spherical accretion on to a point mass has found broad use across fields of astrophysics that were embryonic or non-existent at the time of the paper's publication. In this non-technical review, I describe the motivations for Bondi's work, and briefly discuss some of the applications of Bondi accretion in high energy astrophysics, galaxy formation, and star formation.
