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和文: 
英文:Variability timescale and jet power of 3C 273 
著者
和文: 片岡 淳, 河合 誠之.  
英文: Kataoka, J., Kawai, N..  
言語 English 
掲載誌/書名
和文: 
英文:New Astronomy Review 
巻, 号, ページ Vol. 47        pp. 685-687
出版年月 2003年10月 
出版者
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会議名称
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開催地
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DOI https://doi.org/10.1016/S1387-6473(03)00124-6
アブストラクト We present the results of a long-look monitoring of 3C 273 with RXTE between 1996 and 2000. A total of 230 observations amounts to a net exposure of 845 ks, with this spectral and variability analysis of 3C 273 covering the longest observation period available at hard X-ray energies. Our new observations imply that 3C 273 is a unique object whose hard X-ray emission occasionally contains a component which is not related to a beamed emission (Seyfert like), but most hard X-rays are likely to originate in inverse Compton radiation from the relativistic jet (blazar like). We consider the `power balance' (both radiative and kinetic) between the accretion disk, sub-pc-scale jet, and the 10 kpc-scale jet.

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