This formation, called an accretion disk, may be very important in some stellar birth sequences.
这种构成物即所谓吸积盘, 它在恒星诞生的某些阶段可能是非常重要的.
The Thick Accretion Disk Model and Self - gravitating Accretion Disk Model of QSOs.
类星体的厚吸积盘与自引力吸积盘模型.
The accretion phenomenon was firstly discussed by Kelvin et al. on the 19 th.
十九世纪末,开尔文(Kelvin)等人首先讨论了吸积现象.
When crunched and heated by the black hole's gravitational energy , these disks glow in x - ray light.
吸积盘跟黑洞的引力能之间发生摩擦之后温度升高, 发出 X 射线光.
It is well known that accretion disks are hydrodynamic disks with anomalous viscosity.
天体物理吸积盘是具有反常粘滞的流体盘.
Nevertheless, astrophysicists have persisted in their belief that accretion disks are indeed turbulent.
虽然如此, 天文物理学家仍旧坚持信念,认为吸积盘的确是充满乱流扰动的.
An accretion disk with vertical structure is studied by using a new anomalous viscosity.
利用一种全新的反常粘滞,主要研究了具有垂向结构的吸积盘.
For example, some accretion disks in binary star systems occasionally undergo large, temporary increases in luminosity.
例如, 有些双星系统里的吸积盘,偶尔会短暂地大幅增加亮度.
New material from white dwarf would quickly replenish the blown - apart disk, Strohmayer says.
之后来自快速旋转的白矮星的新物质会迅速地再次充满被吹散的吸积盘, 斯特梅耶说.