A bright millisecond radio burst of extragalactic origin

被引:1469
作者
Lorimer, D. R. [1 ]
Bailes, M.
McLaughlin, M. A.
Narkevic, D. J.
Crawford, F.
机构
[1] W Virginia Univ, Dept Phys, Morgantown, WV 26506 USA
[2] Natl Radio Astron Observ, Green Bank, WV 24944 USA
[3] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[4] Franklin & Marshall Coll, Dept Phys & Astron, Lancaster, PA 17604 USA
关键词
D O I
10.1126/science.1147532
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Pulsar surveys offer a rare opportunity to monitor the radio sky for impulsive burst-like events with millisecond durations. We analyzed archival survey data and found a 30-jansky dispersed burst, less than 5 milliseconds in duration, located 3 degrees from the Small Magellanic Cloud. The burst properties argue against a physical association with our Galaxy or the Small Magellanic Cloud. Current models for the free electron content in the universe imply that the burst is less than 1 gigaparsec distant. No further bursts were seen in 90 hours of additional observations, which implies that it was a singular event such as a supernova or coalescence of relativistic objects. Hundreds of similar events could occur every day and, if detected, could serve as cosmological probes.
引用
收藏
页码:777 / 780
页数:4
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