论文标题
GRB持续时间是否取决于红移？
Does the GRB Duration Depend on Redshift?
论文作者
论文摘要
迄今为止，已经确定了数百个伽马射线爆发（GRB）红移。其他重要属性之一是GRB的距离是爆发的持续时间。在本文中，我们分析了这两个重要数量的现象。在本文中，我们绘制二维分布并探索一些可疑区域。众所周知，短期GRB比其他gr更接近，我们在宇宙中搜索GRB持续时间与其他持续时间不同的部分。我们还分析了红移不同的持续时间中是否有任何范围。我们发现一些可疑区域，但是，除了短期GRB区域，没有其他重要区域。
Several hundred gamma-ray burst (GRB) redshifts have been determined to date. One of the other important properties-besides the distance-of the GRBs is the duration of the burst. In this paper, we analyse these two important quantities of the phenomena. In this paper, we map the two-dimensional distribution and explore some suspicious areas. As it is well known that the short GRBs are closer than the others, we search for parts in the Universe where the GRB duration is different from the others. We also analyse whether there are any ranges in the duration where the redshifts differ. We find some suspicious areas, however, no other significant region was found than the short GRB region.
