Keywords: Astrophysics; X-ray binaries; Neutron stars; Black holes 相似文献
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131.
S.K. Chakrabarti D. Debnath S. Nagarkoti 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(11):3749-3759
The Galactic transient black hole candidate H 1743–322 exhibited a long duration outburst in 2003 after more than two and a half decades of inactivity. The 2003 event was extensively studied in multi-wavelength bands by many groups. The striking feature is that the total energy released is extremely high as compared to that in tens of outbursts which followed. In this paper, we look at this event and study both the spectral and temporal properties of the source using two component advective flow (TCAF) paradigm. We extract accretion flow parameters for each observation from spectral properties of the decay phase and determine the mass of the black hole. We computed the energy released during all the known outbursts since 2003 and showed that on an average, the energy release in an outburst is proportional to the duration of the quiescent state just prior to it, with the exception of the 2004 outburst. A constant rate of supply of matter from the companion cannot explain the energy release in 2004 outburst. However, if the energy release of 2003 is incomplete and the leftover is released in 2004, then the companion’s rate of matter supply can be constant since 1977 till date. We believe that erratic behaviour of viscosity at the accumulation radius of matter as well as location the itself, rather than the random variation of mass transfer rate from the companion, could be responsible for non-uniformity in outburst pattern. We discuss several factors on which the waiting time and duration of the next outburst could depend. 相似文献
132.
E.P.J. van den Heuvel 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2006,38(12):2667-2672
Three recent developments in the field of formation and evolution of neutron stars and black holes in binaries are addressed:
- • The finding that there is a class of neutron stars, formed in interacting binaries, that do not receive kick velocities in their birth events. This finding is particularly important for our understanding of the formation – and formation rates – of double neutron stars. It is argued that these low-kick neutron stars, which tend to have low masses, are formed by a different physical mechanism than the neutron stars that receive large kick velocities at birth.
• The occurrence of velocity kicks in the formation events of stellar black holes.
• The nature of the companions of millisecond X-ray pulsars.
133.
Yu.N. Gnedin 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》1984,3(10-12)
The theory of polarization effects in radiation from compact X-ray sources is presented. The following four problems are considered: 1) the polarization of X-rays from the magnetized neutron stars; 2) the polarization of X-rays from the accretion disk around a black hole; 3) the optical polarization from X-ray binaries, and 4) the results of X-ray polarimetric observations. 相似文献
134.
M. van der Klis 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2004,34(12):2646-2656
Millisecond X-ray time variability studies of accreting low-magnetic-field neutron stars and stellar-mass black holes in X-ray binaries probe the motion of matter in regions of strong gravity. In these regions, general relativity (GR) is no longer a small correction to the classical laws of motion, but instead dominates the dynamics: we are studying motion in strongly curved spacetime. Such millisecond X-ray variability studies can therefore provide unique tests of GR in the strong-field regime. The same studies also constrain neutron-star parameters such as stellar mass and radius, and thereby the equation of state (EOS) of ultradense matter. I briefly review the status, and discuss the prospects for mapping out space-time near accreting stellar-mass compact objects, and measuring the EOS of dense matter, through millisecond timing, particularly with an eye towards future missions. The overwhelming consideration for timing sensitivity is collecting area: contrary to most applications, the signal-to-noise ratio for the aperiodic timing phenomena produced by accretion flows increases proportionally with count rate rather than as the square root of it. A 10 times larger instrument turns 1σ effects into 10σ effects (or does as well in 1% of the time). With the Rossi X-ray Timing Explorer (RXTE), using 0.6 m2 collecting area, we have found several timing diagnostics from the accretion flow in the strong field region around neutron stars and black holes, as well as signals from neutron star surface hot spots. Combined work between RXTE and the new sensitive X-ray spectrographs onboard Chandra and XMM can already begin to clinch the geometry and physical mechanisms underlying these signals. Future instruments, larger in area by an order of magnitude and in some cases with enhanced spectral capabilities, are expected to turn these diagnostics of GR into true tests of GR. They are also expected to put strong constraints on neutron-star structure, and thereby on the EOS of supranuclear density matter. 相似文献
135.
针对低压涡轮叶尖间隙控制系统中典型供气管路,即圆形截面90°弯曲冷却管,开展其工作特性和模拟方法研究.通过1∶1单管模型试验结合三维数值模拟方法,研究了冷却管上冲击孔的出流特性,分析了进气参数、冲击孔排布对冷却管内气体流动及流量分配的影响规律.在此基础上,提出了基于冲击孔进口有效总压概念的冷却管一维网络流动计算模型,建立了低压涡轮叶尖间隙系统中典型供气管路的一维网络流动计算方法,并应用于某型发动机组件流量特性试验设计中.研究中发现,随着远离进口位置,冷却管冲击孔出流流量和冲击孔流量系数逐步增加;随着进口雷诺数的增加,冷却管内冲击孔出流流量均有所增加,而冲击孔流量系数基本保持不变.试验数据和计算结果比对表明,所建立的一维网络流动计算模型可以准确模拟出冷却管的出流特性,计算结果同组件流量特性试验数据之间最大相对误差为4.5%,在叶尖间隙控制系统这类系统复杂流路的流动问题分析中具有良好的应用效果. 相似文献
136.
复合材料开口缝合补强结构力学性能的实验研究 总被引:1,自引:0,他引:1
对复合材料开口缝合补强结构进行了实验研究,测试了不同缝合参数(针距、行距、边距、单重和双重缝合)补强的含孔复合材料层板的破坏强度,研究了孔边应力集中和缝合补强对强度、破坏应变等力学性能参数的影响,分析讨论了孔边及邻近区域应变集中及应变分布的规律,结合破坏断面分析,探讨了不同缝合参数对应变集中及破坏机理的影响,研究结果表明:孔口缝合补强后,层板破坏强度和孔边局部刚度均有增大趋势,孔边产生了\"缺口强化\"现象;与未缝合情况相比,孔边应变衰减范围基本相同,而应变衰减程度不同;缝合设计参数(针距、行距、边距等)不同,孔边拉、压应变的转换点的位置也不同;不同的针距、行距以及边距对孔边应变集中都有很大影响. 相似文献
137.
138.
开孔曲面自动铺放轨迹规划算法研究 总被引:1,自引:0,他引:1
为解决开孔曲面自动铺放轨迹规划问题,提出在前处理中将孔边界内外的曲面接合成完整曲面的方法,采用STL文件提取网格化曲面信息并重构开孔曲面拓扑,按照设定算法获得“连续”的铺放轨迹后,再按孔边对轨迹点进行信息整理得到后置处理所需的最终铺放轨迹点信息.研究了迭代法和投影法在轨迹线与孔边界交点的求取方法,综合比较2种算法的效率和精度后,发现投影法更适于开孔曲面的轨迹规划.根据上述算法,编写了基于VC++ 6.0平台的轨迹规划程序,以整体复合材料前机身为例进行算法验证,证明了提出的开孔曲面自动铺放轨迹规划算法的合理性和正确性. 相似文献
139.
为获得涡轮机匣内部表面换热系数分布数据,以带有加强肋的排孔冲击连腔结构为对象进行了瞬态液晶实验。研究了不同射流雷诺数(Re=5.1×103~1.1×104)、冲击间距比(2.5,5.0,7.5)及轴向间距比(4.0,9.0,14.0)对靶面努塞尔数的影响规律。实验结果表明:增大射流雷诺数对靶面平均努塞尔数的提升最显著。随着冲击间距比的增大,靶面平均努塞尔数逐渐减小,但这种换热削弱效果局限在距冲击驻点2D~3D(D为冲击孔直径)范围内,其它区域的变化很小。在靠近前后端壁的局部区域,表面努塞尔数随冲击间距比的增大而增大。轴向间距比的改变不会影响无出流孔靶面的换热情况,对于有出流孔靶面而言,轴向间距比为9.0的结构换热效果最好。Re=5.1×103条件下,轴向间距比为9.0结构在有出流孔靶面上的平均努塞尔数相比4.0和14.0结构分别增大了5.7%和8.1%,并且随雷诺数增大,增幅越大。 相似文献
140.