Later simulations show that even a companion with an orbit as wide as neptune ' s could scoop up an accretion disk 后来的数值模拟结果显示出，即使伴星的轨道半径大如海王星的轨道，它仍可汲取物质而形成吸积盘。
Although it becomes invisible past a certain point , an accretion disk , which is visible , develops as the matter swirls toward the black hole 虽然它变成看不见的过去某点,一个增大圆盘,是可见的,当物质向黑洞成漩涡发展。
Investigators have conducted laboratory experiments to search for turbulence in flows that resemble accretion disks , but again the results have been debated 研究人员也做实验寻找像吸积盘般流动的乱流，而结果仍有争论。
Although turbulence is sometimes seen in these experiments , it may arise from effects that would not be present in a real accretion disk 虽然有时在这些实验中可看见乱流，但那可能源自某些不会出现在真实吸积盘中的效应。
Because accretion disks also contain flows with very high rates of shear , scientists proposed in the 1970s that the disks must also be highly turbulent 因为吸积盘也包含具有非常高切变率的流体，科学家在1970年代倡议吸积盘必定非常混乱。
By cutting the gordian knot in this way , astrophysicists have been able to build theoretical models of accretion disks to compare with observations of actual disks 用这方法简化难题，天文物理学家就能够建立吸积盘的理论模型，以便与实际圆盘的观测比较。
A black hole can accrete matter into itself as the matter falls or is pulled towards it . the accreting material then orbits around the black hole , forming an accretion disk 当任何物体堕进或被吸入黑洞时，都会被黑洞吸积入内，形成黑洞外的吸积盘绕著黑洞运行。
Such structures , called accretion disks , are also thought to exist around supermassive black holes ( which can weigh as much as a billion suns ) at the centers of galaxies 这种结构称为吸积盘，被认为也存在于星系中心的超大质量黑洞（最重可达10亿倍太阳质量）周遭。
The efficient conversion of mass into energy by friction in the accretion disk of a black hole seems to be the only explanation for the copious amounts of energy generated by such objects 在黑洞增大圆盘片靠摩擦质量有效转化为能量好像只能解释靠这样的物体产生的大量能量。
For neutron stars and black holes , accretion disk will emit high - energy x - rays when matters are spiraling in the compact objects , since immense gravitational force can cause substantial heat up of the matters 对于中子星和黑洞来说，大的重力使吸积盘内物质的温度大幅上升，发出能量很高的x射线。
