radio pulsars的意思|示意
射电脉冲星
radio pulsars的网络常见释义
射电脉冲星 射电脉冲星 (radio pulsars) 1967年剑桥大学穆拉德射电天文台研究生Jocelyn Bell 利 用A.
radio pulsars相关例句
Since their discovery in 1967 by Jocelyn Bell and Anthony Hewish in Cambridge, UK, radio pulsars are one of the most exciting fields of astronomical research.
自从1967年由英国剑桥大学的Jocelyn Bell和Anthony Hewish发现了射电脉冲星后,射电脉冲星已经成为天文学中最激动人心的研究领域之一。
But certain stars, called pulsars, give off regular pulses of radio waves.
但有些恒星,所谓的脉冲星,会有规律地发出射电波脉冲。
Also on display for the first time is a section of the radio telescope which radio astronomer Jocelyn Bell used to discover pulsars - small, fast-rotating stars - in the 1960s.
展览还首次展出了20世纪六十年代射电天文学家Jocelyn Bell发现高速运转的小恒星-脉冲星时所使用的射电望远镜。
The solution emerged from an entirely separate line of work, on radio pulsars.
问题的答案,得从另一条完全不相同的思路中寻找:无线电波霎。
The extension of astronomy from visible light to radio waves to x-rays and gamma rays never failed to lead to the discovery of unusual objects such as radio galaxies, quasars, and pulsars.
从可见光扩展到无线电波,再到 X 射线和伽马射线,天文学总是会发现不寻常的物体,如射电星系、类星体和脉冲星。
Radio pulsars are neutron stars with an immensely strong magnetic field.
射电脉冲星是带有强磁场的中子星。