有許多的高質量X射線雙星（highmass Xray binary）的光學對應體尚未被認定。高質量X射線雙星在近紅外線波段有特別的顏色分佈，我們預期光學對應體尚未被認定的高質量X射線雙星會符合這個近紅外線波段的顏色分佈。我們利用高質量X射線雙星目錄比對其二微米全天巡天計畫（2MASS）和Spizter遺跡計畫中的GLIMPSE紅外資料去搜尋尚未被認定出光學對應體的高質量X射線雙星。我們找出一些在之前尚未被認定光學對應體的高質量X射線雙星的候選者，其中有一些很有可能就是高質量X射線雙星的光學對應體。我們列出這些候選者，並對我們的結果進行討論。 Optical counterparts of many high mass X-ray binaries are not identified. The high mass X-ray binaries have characteristic colors at near infrared. We expect that most of the unidentified high mass X-ray binaries should also show similar infrared characteristics. We thus use the catalog of high mass X-ray binaries to search for their near-infrared counterparts in 2MASS and Spitzer legacy program-GLIMPSE data archive. We have identified some probable counterparts and found potential candidates for most of the previously unidentified high mass X-ray binaries. We present a catalog of these candidates and discuss our results.
