In the prothallial and sporogonium period,their feature isozymes bands appeared stably.
不同发育期,均有特征带。
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A remnant that has an unusually strong magnetic field could produce radio emissions, and as it is not a neutron star, it could get away with being as slow and stably rotating as the source of GPM J1839–10 while doing so.
具有异常强磁场的遗迹可能会产生无线电发射,而且由于它不是中子星, 因此在这样做时它可能会像 GPM J1839-10 的源一样缓慢而地旋转。