Observational Constraints on Radiatively Inefficient Accretion Flows in Nearby AGNs(Poster)
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概要
- 論文の詳細を見る
Results of recent X-ray observations of low-luminosity AGNs are summarized. The lack of the signature of X-ray reflection features and big blue bump is in good agreement with the prediction that an optically thick accretion disk is truncated. Comparison of radio and X-ray luminosities indicates that low-luminosity objects tend to be radio loud compared to more luminous AGNs, suggesting efficient jet production in low-luminosity accretion flows.
- 理論物理学刊行会の論文
- 2004-11-15
著者
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Yamagami Takamasa
Institute Of Space And Astronautical Science
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Terashima Yuichi
Institute Of Space And Astronautical Science
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