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Einstein@Home discovers a radio-quiet gamma-ray millisecond pulsar

机译:爱因斯坦@霍姆发现无线电波静默的伽马射线毫秒脉冲星

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摘要

Millisecond pulsars (MSPs) are old neutron stars that spin hundreds of times per second and appear to pulsate as their emission beams cross our line of sight. To date, radio pulsations have been detected from all rotation-powered MSPs. In an attempt to discover radio-quiet gamma-ray MSPs, we used the aggregated power from the computers of tens of thousands of volunteers participating in the Einstein@Home distributed computing project to search for pulsations from unidentified gamma-ray sources in Fermi Large Area Telescope data. This survey discovered two isolated MSPs, one of which is the only known rotation-powered MSP to remain undetected in radio observations. These gamma-ray MSPs were discovered in completely blind searches without prior constraints from other observations, raising hopes for detecting MSPs from a predicted Galactic bulge population.
机译:毫秒脉冲星(MSP)是古老的中子星,每秒旋转数百次,并且在其发射束穿过我们的视线时似乎在脉动。迄今为止,已经从所有旋转供电的MSP中检测到无线电脉冲。为了发现安静的伽马射线MSP,我们利用来自参与Einstein @ Home分布式计算项目的成千上万名志愿者的计算机的合计功率来搜索费米大区域中来自身份不明的伽马射线源的脉动望远镜数据。这项调查发现了两个孤立的MSP,其中之一是在无线电观测中未被发现的唯一已知的旋转动力MSP。这些伽马射线MSP是在完全盲目搜索中发现的,而没有其他观测结果的事先限制,这为从预测的银河膨胀种群中检测MSP带来了希望。

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