Those observations have revealed that SN 1979c has not dimmed in the 31 years since its birth, as would be expected if this was anything less than a genuine black hole.

这些观察结果透露了SN 1979c从它出生后的31年里还没有暗淡下去，可以想象，如果说有任何不同，都比不上一个真正的黑洞那样激动人心。

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This would make the object in SN 1979c the youngest and brightest example of such a "pulsar wind nebula" and the youngest known neutron star.

如果是这样的话，SN 1979c中的这个天体将是迄今为止观测到的最年轻最明亮的“脉冲风星云”，是已知最年轻的中子星。

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What makes this one -- dubbed SN 1979C -- special is that it has been observed over the years with a series of orbiting x-ray telescopes, most lately the Chandra X-Ray Observatory.

使得这个天体（被称为SN 1979C）如此特别的事实在于多年以来它已经被一系列轨道上的X射线望远镜所观察研究，最近的观测是钱德拉X射线天文台所做的。

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Formally called SN SCP-0401, the supernova was something of a chance find in a survey carried out in part by the Supernova Cosmology Project (SCP) using the Hubble space telescope, first undertaken in 2004.

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