论文标题
一个近似值来确定哇的来源！信号
An approximation to determine the source of the WOW! Signal
论文作者
论文摘要
在本文中，可以分析《魔兽世界》中成千上万的恒星中的哪一颗！信号区域可能是信号真正来源的最高机会，只要它来自类似于我们的星系。采样了总共66 g和K型星，但考虑到Gaia档案中的可用信息，只有一个被确定为潜在的类似太阳的恒星。因此，该候选资源称为2MASS 19281982-2640123，因此成为进行观察的理想目标，以寻找潜在的可居住系外行星。另外两个候选恒星具有亮度误差间隔，其中包括太阳的光度，还有14个候选者也被确定为潜在的类似太阳的恒星，但对其光度的估计尚不清楚。
In this paper it is analysed which of the thousands of stars in the WOW! Signal region could have the highest chance of being the real source of the signal, providing that it came from a star system similar to ours. A total of 66 G and K-type stars are sampled, but only one of them is identified as a potential Sun-like star considering the available information in the Gaia Archive. This candidate source, which is named 2MASS 19281982-2640123, therefore becomes an ideal target to conduct observations in the search for potentially habitable exoplanets. Another two candidate stars have a luminosity error interval that includes the luminosity of the Sun, and 14 candidates more are also identified as potential Sun-like stars, but the estimations on their luminosity were unknown.
