Interactions and Collisions of Stars and Pulsars, and the Magnetic Fields of Early Star Formation

恒星和脉冲星的相互作用和碰撞，以及早期恒星形成的磁场

• 批准号: 9618537
• 负责人: E. Sterl Phinney
• 金额: $ 18.4万
• 依托单位: California Institute of Technology
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1997
• 资助国家: 美国
• 起止时间: 1997-06-01 至 2000-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9618537&HistoricalAwards=false
• 关键词: Interactions; Collisions; Stars; Pulsars; Magnetic

Phinney, E. Sterl AST 96-18537 Dr. Phinney will carry out a program of theoretical research on a diverse array of topics related by the general theme of the physics of compact objects and magnetic fields in young galaxies. His research program has three major goals : 1) to investigate the ways in which binary stars can interact with each other through both gravitational and non-gravitational forces, 2) to improve understanding of the ways in which pulsars lose energy and the properties of their winds and magnetospheres, and 3) to develop techniques for determining the origin of the magnetic fields in galaxies and clusters. ***

Phinney，E. Sterl AST 96-18537 Phinney博士将开展一项理论研究计划，涉及各种主题， 年轻星系中致密物体和磁场的物理学主题。 他的研究计划有三个主要目标：1）调查双星如何 通过重力和非重力相互作用，2）改善 了解行星失去能量的方式和它们的风的性质， 磁层，以及3）开发用于确定磁场起源的技术， 星系和星系团 ***