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81.
The broad X-ray iron line observed in many active galactic nuclei spectra is thought to originate from the accretion disc surrounding the putative supermassive black hole. We show here how to perform the analytical integration of the geodesic equations that describe the photon trajectories in the general case of a rotating black hole (Kerr metric), in order to write a fast and efficient numerical code for modelling emission line profiles from accretion discs. 相似文献
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Johan G. Borchert 《GeoJournal》1998,45(4):327-336
The retail system is continuously adapting itself to changing demographic conditions, consumer behavior and economic conditions.
Existing retail units, getting larger in order to achieve economics of scale, and new forms of large-scale retailing do not
fit easily in the traditional spatial pattern of retail concentrations. Neverteless the spatial distribution of retailing
in urban areas, as schematized by Berry thirty-five years ago, still has its value. Through an upward hierarchical movement
the retail system has adapted itself to an inflexible spatial system, in which downtown has still a dominant position. Future
developments, however, may weaken the position of central shopping areas in favour of peripheral locations.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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It is known that a sharp decrease in the angular velocity of the accretion disk around a black hole could in principle produce a kinematic axisymmetric dynamo, in contrast to the classical situation described by Cowling's antidynamo theorem. Here the effect of a nontrivial poloidal velocity of the disk is studied, showing that a strong gradient of this velocity enhances the possibilities of a working dynamo. 相似文献
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本文用样条函数法实现了二维位场的向上延拓和向下延拓,向上延拓用样条函数法计算泊松积分,向下延拓用样条函数法求解第一类Fredholm积分方程。模型和实例计算表明,本文方法正确可行且精度高。 相似文献
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查明浅表部地层地质条件,对多层及高层建筑均至关重要。针对目前上海地区,在运用小螺纹钻孔进行浅表部工程勘察中存在的一些问题,就其如何合理使用,作了若干方面的探讨。 相似文献
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We examine the status of the threat posed to stellar-mass black hole candidates by the possible existence of Q-stars (compact objects with an exotic equation of state that might have masses well above the normally accepted maximum for standard neutron stars). We point out that Q-stars could be extremely compact (with radii less than 1.5 times the corresponding Schwarzschild radius) making it difficult to determine observationally that a given object is a black hole rather than a Q-star, unless there is direct evidence for the absence of a material surface. On the other hand, in order for a Q-star to have a mass as high as that inferred for the widely favoured black hole candidate V404 Cygni, it would be necessary for the Q-matter equation of state to apply already at densities an order of magnitude below that of nuclear matter and this might well be considered implausible on physical grounds. We also describe how rotation affects the situation and discuss the prospects for determining observationally that black hole candidates are not Q-stars. 相似文献