| DC 欄位 |
值 |
語言 |
| DC.contributor | 天文研究所 | zh_TW |
| DC.creator | 洪子隆 | zh_TW |
| DC.creator | Tzu-Lung Hung | en_US |
| dc.date.accessioned | 2005-7-24T07:39:07Z | |
| dc.date.available | 2005-7-24T07:39:07Z | |
| dc.date.issued | 2005 | |
| dc.identifier.uri | http://ir.lib.ncu.edu.tw:88/thesis/view_etd.asp?URN=92229013 | |
| 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 | 我們使用了活躍星系核 (active galactic nuclei，簡稱為AGNs) 在靜止座標之下紫外波段連續譜與其寬發射線區域 (broad line region，簡稱為BLR) 尺度的關係，計算了93個高紅移 (2.5| zh_TW | |
| DC.subject | 類星體 | zh_TW |
| DC.subject | 艾丁吞吸積率 | zh_TW |
| DC.subject | 鮑德溫效應 | zh_TW |
| DC.subject | Baldwin Effect | en_US |
| DC.subject | Eddington Ratio | en_US |
| DC.subject | QSOs | en_US |
| DC.title | 高紅移類星體的艾丁吞吸積率及鮑德溫效應 | zh_TW |
| dc.language.iso | zh-TW | zh-TW |
| DC.title | The Eddington Ratio and Baldwin Effect of High Redshift QSOs | en_US |
| DC.type | 博碩士論文 | zh_TW |
| DC.type | thesis | en_US |
| DC.publisher | National Central University | en_US |