| DC 欄位 |
值 |
語言 |
| DC.contributor | 天文研究所 | zh_TW |
| DC.creator | 黃國斌 | zh_TW |
| DC.creator | Kuo-Pin Huang | en_US |
| dc.date.accessioned | 2007-7-17T07:39:07Z | |
| dc.date.available | 2007-7-17T07:39:07Z | |
| dc.date.issued | 2007 | |
| dc.identifier.uri | http://ir.lib.ncu.edu.tw:88/thesis/view_etd.asp?URN=942209003 | |
| dc.contributor.department | 天文研究所 | zh_TW |
| DC.description | 國立中央大學 | zh_TW |
| DC.description | National Central University | en_US |
| dc.description.abstract | 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。 | zh_TW |
| dc.description.abstract | 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. | en_US |
| DC.subject | 光學對應體 | zh_TW |
| DC.subject | 高質量X射線雙星 | zh_TW |
| DC.subject | 近紅外波段 | zh_TW |
| DC.subject | near infrared | en_US |
| DC.subject | high-mass x-ray binaries | en_US |
| DC.subject | counterpart | en_US |
| DC.title | 使用近紅外波段搜尋高質量X射線雙星的光學對應體 | zh_TW |
| dc.language.iso | zh-TW | zh-TW |
| DC.title | Search for Counterpart of High-Mass X-ray Binaries at Near Infrared | en_US |
| DC.type | 博碩士論文 | zh_TW |
| DC.type | thesis | en_US |
| DC.publisher | National Central University | en_US |