期刊文献+

FAST——脉冲星观测研究的利器 被引量:6

FAST: A sharp tool to do pulsar studies
原文传递
导出
摘要 2016年9月25日落成的中国自行设计建造的500 m口径球面射电望远镜(FAST)是目前全世界最大口径的射电望远镜。在调试期间已成功发现了脉冲星,实现了国内设备发现脉冲星的零突破。脉冲星是宇宙中的一类奇妙天体,是验证强引力场、强磁场和高密度等极端物理环境下物理规律的"天然实验室"。作为脉冲星研究的利器,预计FAST大规模巡天能够大幅提高已知的脉冲星数目。FAST还将在低频引力波探测、脉冲星物理、星际和星系际介质探测、脉冲星时间尺度建立及脉冲星导航等领域取得突破性进展。在上述研究中,国内天文设备取长补短、相互补充,有望实现中国脉冲星观测研究跨越式发展。 The Five-hundred-meter Apemue Spherical Radio Telescope(FAST), which is independently designed and built in China, is the largest single-dish telescope on the earth.The construction was completed on September 25th, 2016. A few new pulsars were discovered by the FAST during its commissioning phase, as the first pulsar discovery with the telescope in China. The pulsar is a fantastic object, which serves as the natural lab on the sky for studies of the extreme physical conditions, including the strong gravitational field, the strong magnetic field and the high density. The FAST is a very useful tool for pulsar studies, and can make breakthro-o-hs in the following areas: boosting the pulsar number, detecting gravitational wave, studying the interstellar and intergalactic medium, building the pulsar timesca/e and the deep space navigation system, and others. In the field of pulsar research, all kinds of telescopes may play a role, and it can be anticipated that with the addition of the FAST, the domestic pulsar research will have a leap forward.
作者 闫振 沈志强
出处 《科技导报》 CAS CSCD 北大核心 2017年第24期16-19,共4页 Science & Technology Review
基金 国家自然科学基金项目(11403073 U1631122 11633007) 中国科学院B类战略性先导科技专项(XDB23010200)
关键词 射电望远镜 脉冲星 引力波 星际介质 星系际介质 radio telescope pulsar , gravitational wave interstellar medium intergalactic medium
  • 相关文献

参考文献8

二级参考文献71

  • 1韩金林.银河系磁场的研究[J].自然杂志,2007,29(2):96-101. 被引量:2
  • 2[2]Taylor J H.Millisecond pulsars:Nature's most stable clocks[C]//Proceedings of the IEEE,Las Vegas,Nevada,July 1991:1054 -1062 被引量:1
  • 3[3]Pines D J.ARPA/DARPA Space Programs[M].XNAV Industry Day,Aug.2004:1-15 被引量:1
  • 4[4]Sheikh S I,Pines D J,et al.The use of X-ray pulsar for spacecraft navigation[C]//Proceedings of the 14th AAS/AIAA Space Flight Mechanics Conference,AAS 04-109,Maui,HI,Feb.2004:105-119 被引量:1
  • 5[5]Hellings R W.Relative effects in astronomieal timing measurements[J].Astronomical Journal,March 1986,91:650-659 被引量:1
  • 6[8]Brown R G,Hwang P Y C.Introduction to Random Signals and Applied Kalman Filtering[M].Published by John Wiley & Sons,Inc.,New York,1997:419-460 被引量:1
  • 7Hewish A, Bell S J, Pilkington, et al. Nature, 1968, 217:709. 被引量:1
  • 8Levinovitz A W, Ringertz N. The Nobel Prize: the first 100 years, London: Imperial College Press, 2001. 被引量:1
  • 9Lyne A G, Lorimer D R. Nature, 1994, 369:127. 被引量:1
  • 10Chatterjee S, Vlemmings W H T, Brisken W F, et al. ApJ, 2005, 630:61. 被引量:1

共引文献80

同被引文献51

引证文献6

二级引证文献22

相关作者

内容加载中请稍等...

相关机构

内容加载中请稍等...

相关主题

内容加载中请稍等...

浏览历史

内容加载中请稍等...
;
使用帮助 返回顶部