摘要
通过比较不同观测中Ｇｅｍｉｎｇａ脉冲星的γ射线绝对位相，测量出了不同时间Ｇｅｍｉｎｇａ的位置。这些位置表明Ｇｅｍｉｎｇａ自行的赤经分量为０．２２６±０．０３弧秒／年，与它的一个最可能的光学对应体Ｇ″的自行相一致，从而独立地确定了Ｇ″与Ｇｅｍｉｎｇａ之间的对应关系。
We have measured the right ascension of Geminga at different epochs by comparing the absolute phases between the different γ-ray observations.These values show that the right-ascension component of the proper motion of Geminga is 0.226±0.03 arcsec per year, which is consistent with that of G″, the most probable optical counterpart, thus independently confirming the correspondence between G″and Geminga.
