Formation of Black Hole Relativistic Jets at Low Accretion Rate
博士 === 國立清華大學 === 物理系 === 101 === Observed correlations between the disk luminosity (L) and radio emission from accreting black hole (BH) systems indicate underlying couplings between BH accretion disk and jet. Assuming relativistic jets are launched at the expense of the rotational energy of spinni...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2013
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| Online Access: | http://ndltd.ncl.edu.tw/handle/23785944085880375113 |