使用近紅外波段搜尋高質量X射線雙星的光學對應體; Search for Counterpart of High-Mass X-ray Binaries at Near Infrared

Please use this identifier to cite or link to this item: http://ir.lib.ncu.edu.tw/handle/987654321/6102

Title:	使用近紅外波段搜尋高質量X射線雙星的光學對應體;Search for Counterpart of High-Mass X-ray Binaries at Near Infrared
Authors:	黃國斌;Kuo-Pin Huang
Contributors:	天文研究所
Keywords:	光學對應體;高質量X射線雙星;近紅外波段;near infrared;high-mass x-ray binaries;counterpart
Date:	2007-06-21
Issue Date:	2009-09-22 10:13:15 (UTC+8)
Publisher:	國立中央大學圖書館
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。 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.
Appears in Collections:	[Graduate Institute of Astronomy] Electronic Thesis & Dissertation

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