在活躍星系核OH-010的噴流中檢測絕熱膨脹與能量均分兩噴流模型
碩士 === 國立清華大學 === 物理系 === 102 === The quasar OH-010 is studied using data obtained by the Very Long Baseline Array (VLBA)at 15.4 GHz from the MOJAVE (Monitoring Of Jets in Active galactic nuclei with VLBA Experiments) archive and light curves from single dish observations at 4.8, 8, 14.5, 22, 37,and...
| Main Authors: | , |
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| Format: | Others |
| Language: | en_US |
| Published: |
2014
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| Online Access: | http://ndltd.ncl.edu.tw/handle/00780444784718443429 |