A simple mass estimate for central black holes in cuspy galaxies     

Herwig Dejonghe  Anne Mathieu  Veronique De Bruyne  Sven De Rijcke 《Celestial Mechanics and Dynamical Astronomy》1998,72(3):219-233

We argue that the temperature of the stellar phase is likely a monotically decreasing function of radius in the central regions of elliptical galaxies with cusps. We show that it requires the presence of a central mass concentration. An estimate of its minimum mass based on few parameters is given. This lower bound is consistent with current mass values of the central objects in galaxies derived from detailed models. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

High-redshift galaxies, their active nuclei and central black holes     

Martin G. Haehnelt  Priyamvada Natarajan  & Martin J. Rees 《Monthly notices of the Royal Astronomical Society》1998,300(3):817-827

We demonstrate that the luminosity function of the recently detected population of actively star-forming galaxies at redshift z  = 3 and the B -band luminosity function of quasi-stellar objects (QSOs) at the same redshift can both be matched with the mass function of dark matter haloes predicted by standard variants of hierarchical cosmogonies for lifetimes of optically bright QSOs anywhere in the range 10⁶ to 10⁸ yr. There is a strong correlation between the lifetime and the required degree of non-linearity in the relation between black hole and halo mass. We suggest that the mass of supermassive black holes may be limited by the back-reaction of the emitted energy on the accretion flow in a self-gravitating disc. This would imply a relation of black hole to halo mass of the form M _bh ∝  v ⁵_halo ∝  M ^5/3_halo and a typical duration of the optically bright QSO phase of a few times 10⁷ yr. The high integrated mass density of black holes inferred from recent black hole mass estimates in nearby galaxies may indicate that the overall efficiency of supermassive black holes for producing blue light is smaller than previously assumed. We discuss three possible accretion modes with low optical emission efficiency: (i) accretion at far above the Eddington rate, (ii) accretion obscured by dust, and (iii) accretion below the critical rate leading to an advection-dominated accretion flow lasting for a Hubble time. We further argue that accretion with low optical efficiency might be closely related to the origin of the hard X-ray background and that the ionizing background might be progressively dominated by stars rather than QSOs at higher redshift.  相似文献   

Line emission from accretion discs around black holes: the analytic approach     

Andrej ?ade?  Claudio Fanton  Massimo Calvani 《New Astronomy》1998,3(8):528-654

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   

钻进过程孔内动态参数同步采集系统的研制   总被引：3，自引：1，他引：2       下载免费PDF全文

补家武  龚元明  吴翔 《探矿工程》1998,(1):29-30

介绍了钻进过程孔内参数采集系统的组成原理,性能指标与特点,试验情况和应用前景。  相似文献   

武汉白沙洲长江大桥百米长桩成孔技术与施工实践          下载免费PDF全文

李世京  廖光华 《探矿工程》1998,(3):10-11

介绍了百米长桩的施工方法、施工设备、护孔技术,并就深孔实施泵吸反循环的可行性、主要技术措施以及强风化岩层的糊钻问题进行了分析。  相似文献   

松花江水下爆破孔施工技术          下载免费PDF全文

赵大军  徐龙献  陈宝义 《探矿工程》1998,(4):12-14

在东北严寒季节,在松花江上施工水下爆破孔。介绍了施工设备及施工平台,根据不同地层分别采用静压振动下套管护壁及潜孔锤钻进方法,设计了风路系统,改进了套管妆方法,并采取了科学的管理方法,取产好的效果。  相似文献   

Kinematic Dynamos in the Kerr Metric     

Núñez  M. 《Studia Geophysica et Geodaetica》1998,42(3):424-430

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   

钻孔雷达定向测量技术与应用   总被引：3，自引：1，他引：2  

南生辉 《煤田地质与勘探》1998,(Z1)

介绍了钻孔雷达定向测量技术的原理,结合实例说明资料解释方法及探测效果。  相似文献   

浅表地质现象对工程建设的影响及其勘探技术     

冯铭璋 《上海国土资源》1998,(3)

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   

Are Q-stars a serious threat for stellar-mass black hole candidates?     

Miller  Shahbaz  & Nolan 《Monthly notices of the Royal Astronomical Society》1998,294(2):L25-L29

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