论文标题
病毒云解释银河系中的旋转不对称性
Virial clouds to explain rotational asymmetry in galactic halos
论文作者
论文摘要
通过CMB数据中的非对称多普勒移位可以看到银河对象的旋转。在病毒温度下的分子氢云可能有助于银河系黑物质，这可能是在银河系光环中观察到的旋转不对称的原因。我们提出了一种约束这些病毒云参数的方法，因为它们是由单个流体组成的。该方法应该可以将其扩展到多种流体。
The rotation of the galactic objects has been seen by asymmetric Doppler shift in the CMB data. Molecular hydrogen clouds at virial temperature may contribute to the galactic halo dark matter and they might be the reason for the observed rotational asymmetry in the galactic halos. We present a method to constrain the parameters of these virial clouds given that they are composed of a single fluid. The method is such that it should be possible to extend it to more than one fluid.
