Radio Pulsars: Precession, Planets and Kinematics

射电脉冲星：进动、行星和运动学

• 批准号: 9218075
• 负责人: James Cordes
• 金额: $ 23.33万
• 依托单位: Cornell University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1993
• 资助国家: 美国
• 起止时间: 1993-03-15 至 1996-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9218075&HistoricalAwards=false
• 关键词: Radio; Pulsars; Precession; Planets; Kinematics

Observational studies related to pulsars will be undertaken. Pulse timing and shape data will be used to study variations in the pulse periods with the goal of separating various effects and ascertaining whether the presence of companions can be demonstrated. Proper motion measurements will be made to place constraints of formation processes and searches will be made for new pulsars both in the radio and infrared spectral regions. The search may uncover a new class of pulsars.

将进行与脉冲星有关的观测研究。脉冲时间和形状数据将用于研究脉冲周期的变化，目的是分离各种影响，并确定是否可以证明伴星的存在。将进行适当的运动测量，以确定形成过程的限制，并将在无线电和红外光谱区域搜索新的脉冲星。这项研究可能会发现一类新的脉冲星。