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2009年11月11日,正在新加坡参加亚太经合组织领导人会议周活动的世界银行行长佐利克说:如果美国不能很好地处理贸易和财政"双赤字"问题,美元就有可能失去世界主要储备货币的地位.他说:美元能够成为世界主要储备货币,是美国用了约200年的辛苦努力换来的.他还说:鉴于中国经济增长趋势和中国为使人民币国际化所做的努力,未来15年内,人民币有可能成为代替美元的国际储备货币之一. 相似文献
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Ya-Di Xu Xin-Wu Cao 《中国天文和天体物理学报》2009,9(4)
It was found that advection-dominated accretion flow (ADAF)+thin disk model calculations can reproduce the observed spectral energy distributions (SEDs) of two low- luminosity active galactic nuclei (AGNs), provided they are accreting at ~ 0.01 - 0.03 Eddington rates and the thin disks are truncated to ADAFs at~ 100Rs (Rs is the Schwarzschild radius) for M81 and NGC 4579 (Quataert et al. 1999). However, the black hole masses adopted in their work are about one order of magnitude lower than recent measurements on these two sources. Adopting the well estimated black hole masses, our ADAF+thin disk model calculations can reproduce the observed SEDs of these two low- luminosity AGNs, if the black hole is accreting at 2.5 × 10-4 Eddington rates with the thin disk truncated at Rtr = 120Rs for M81 ((m) = 3.3 × 10-3 and Rtr = 80Rs are required for NGC 4579). The transition zones with temperature from the thin disk with 104 - 105 to~109 - 1010 K in the ADAF will inevitably emit thermal X-ray lines, which provides a useful diagnosis of their physical properties. The observed widths of the thermal X-ray iron lines at(~)6.8 keV are consistent with Doppler broadening by Keplerian motion of the gases in the transition zones at~100Rs. We use the structure of the transition zone between the ADAF and the thin disk derived by assuming the turbulent diffusive heat mechanism to calculate their thermal X-ray line emission with the standard software package Astrophysical Plasma Emission Code (APEC). Comparing them with the equivalent widths of the observed thermal X-ray iron lines in these two sources, we find that the turbulent diffusive heat mechanism seems to be unable to reproduce the ob- served thermal X-ray line emission. The test of the evaporation model for the accretion mode transition with the observed thermal X-ray line emission is briefly discussed. 相似文献