Since then, several other binary pulsars have been found, in particular the double pulsar PSR J0737-3039, in which both stars are pulsars.
更重要的是,这次研究的脉冲星每分钟可以旋转150次。
What's more, the pulsar in our study spins 150 times every minute.
这14个被确认为创造地球地图的物体确实是脉冲星,所以这个计划看起来很不错。
These 14 objects identified to create an Earth-finding map are indeed pulsars, and so the plan seemed like a good one.
在J1023中,恒星足够接近,气流从太阳状恒星流向脉冲星。
In J1023, the stars are close enough that a stream of gas flows from the sun-like star toward the pulsar.
这些包括恒星和星系,以及全新的天体种类,如電波星系,类星体,脉冲星和微波激射器。
These include stars and galaxies, as well as entirely new classes of objects, such as radio galaxies, quasars, pulsars, and masers.
J0740+6620是一种旋转中子星,也被称为脉冲星。
J0740+6620 is a kind of rotating neutron star known as a pulsar.
费米LAT与中国FAST之间的合作关系显着提高了科学家探测最微弱的脉冲星的能力,称为毫秒脉冲星。
The partnership between Fermi LAT and China's FAST significantly improves the ability of scientists to detect the faintest pulsars, called millisecond pulsars.
年、2006年、2009年和2016年的钱德拉数据显示了脉冲星风星云随时间发生的变化。
The Chandra data taken in 2000, 2006, 2009, and 2016 show changes in the pulsar wind nebula with time.
在此阶段之后,由于团队尚不了解的原因,脉冲星短暂再次明亮了约20%。
Following this phase, the pulsar briefly brightened again by roughly 20 percent for reasons the team does not yet understand.
要知道从10亿选出14个将是一项艰巨的任务,因为脉冲星周期并不是唯一的。
To know which 14 are chosen out of one billion will be a daunting task, since pulsar periods are not unique.
这项为期14年的实验还为脉冲星本身的物理机制提供了令人兴奋的新信息。
The 14-year-long experiment also provided exciting insight into the little-understood workings of pulsars themselves.
脉冲星轨道衰减的测量显示它们失去的能量与广义相对论预测的数据一致。
Measurements of the orbital decay of the pulsars showed they lost energy matching the amounts predicted by general relativity.
数据集越长,脉冲星定时技术就越强大,”科尔说。
The longer the data set, the more powerful the pulsar timing technique is,” said Kerr.
引力波可以影响脉冲星的射电信号抵达地球所花费的时间。
These waves affect the time it takes for radio signals from pulsars to arrive at Earth.
脉冲星PSRJ1824-2452I和它的伴星的艺术家印象图。
An artist's impression of the pulsar PSR J1824-2452I and its companion star.
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