Neutron Star and Pulsar Studies

中子星和脉冲星研究

• 批准号: 9528435
• 负责人: Shrinivas Kulkarni
• 金额: $ 54万
• 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: 1996
• 资助国家: 美国
• 起止时间: 1996-08-01 至 1999-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9528435&HistoricalAwards=false
• 关键词: Neutron; Star; Pulsar; Studies

95-28435 Kulkarni Dr. Kulkarni's research program includes the application of supercomputers to pulsar searches and an aggressive multi- wavelength observational program, emphasizing radio observations followed by ground-based optical and IR, as well as X-ray observations from satellites. The observational thrusts are: sensitive searches for pulsars in supernova remnants, large blind searches with sensitivity to sub-millisecond pulsars, targeted observations of promising pulsar candidates identified by continuum radio observations, deep searches of globular clusters for millisecond pulsars, sensitive optical/IR observations of binary pulsar systems, multi- wavelength studies of soft gamma-ray repeaters. and attempts to detect radio emission from gamma-ray burst sources. ***

95-28435库尔卡尔尼博士的研究计划包括将超级计算机应用于脉冲星搜索和积极的多波长观测计划，重点是射电观测以及随后的地面光学和红外观测，以及来自卫星的X射线观测。观测任务包括：对超新星遗迹中的脉冲星进行灵敏的搜索，对亚毫秒脉冲星的敏感度进行大规模盲目搜索，对通过连续射电观测确定的有希望的脉冲星候选星进行定向观测，对球状星团进行毫秒脉冲星的深度搜索，对双星脉冲星系统进行灵敏的光学/红外观测，对软伽马射线中继器进行多波长研究。并尝试检测来自伽马射线爆发源的无线电发射。***