SN 1979C

The results seen in the observations of SN 1979C fit this theory very well .

该观点在SN1979C身上得到了充分证明。

, we consider SN 1979c should be classified to type II supernova with some special characteristics .

根据这颗超新星的光变曲线、在星系中的位置及爆发期间辐射的总能量等主要特征，我们认为SN1979c是某些性质比较特殊的II型超新星。

A photographic observation on Sn 1979C in NGC 4321

NGC4321中超新星1979c的照相研究

However , SN 1979C is different because it is much closer and belongs to a class of supernovas unlikely to be associated with a GRB .

但是SN1979C独一无二的是它离我们非常近，而且本该归属于超新星范围，不应该产生伽马线暴。

The 30-year-old object is a remnant of SN 1979C , a supernova in the galaxy M100 approximately 50 million light years from Earth .

这个30岁的物体*是SN1979C超新星爆炸以后的遗留物，它位于M100星系，距地球大约500万光年。

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 .

该假设总结出SN1979C中的物体为最年轻和最明亮的“脉冲波霎星云”和已知最年轻的中子星。

who led the study . The scientists think SN 1979C , first discovered by an amateur astronomer in 1979 , formed when a star about 20 times more massive than the sun collapsed .

SN1979C是由一位业余天文爱好着于1979年首次发现，科学家认为它是由一颗质量比太阳大20倍的恒星坍塌后形成的。

Although the evidence points to a newly formed black hole in SN 1979C , another intriguing possibility is that a young , rapidly spinning neutron star with a powerful wind of high energy particles could be responsible for the X-ray emission .

虽然证据显示SN1979C形成的是一个新兴黑洞，另外一个有趣的假设认为，它可能是一个年轻的，快速旋转的中子星，强大的波云风抛射出高能量粒子也可能产生强x射线。