1.
Extrinsic AGB Stars on Wind Accretion Binary Evolution Model
星风吸积双星演化模型下的外赋AGB星
2.
In the same way, ultraviolet photons from accretion disks around white dwarfs and in active galactic nuclei or quasars may also accelerate winds from the disk.
同样地，来自白矮星、跃星系核或类星体吸积盘的紫外光光子，或许也能够加速从圆盘吹出的风。
3.
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
4.
Accretion Disk and Angular Momentum Loss During Formation of a Star in the Nebular Disk
吸积盘与恒星在星云盘中形成时的角动量损失
5.
The Mass Accretion and Yields of r-process in the s+r Stars;
s+r星的r-过程物质吸积及产量估计
6.
Accretion and Jet Physics in Low Luminosity Active Galactic Nuclei;
低光度活动星系核的吸积和喷流研究
7.
Mass Accretion Parametric Model of Extrinsic AGB Stars
物质吸积的外赋AGB星参数化模型
8.
The Effect of Mass Accretion on Elemental Abundances of Metal-Poor Extrinsic AGB Stars;
物质吸积对贫金属外赋AGB星元素丰度的影响
9.
An increase in the mass of a celestial object by the collection of surrounding interstellar gases and objects by gravity.
吸积，天体增大因重力吸引星际间的物质而引起天体的增大
10.
The village was snowed in for more than two weeks after the heavy storm.
暴风雪之后村子被积雪封困了两个多星期。
11.
( Dwarf novae, explosions of light from the accretion disk around a white dwarf in a binary system, are examples of this phenomenon.
在双星系统中，环绕白矮星的吸积盘产生光爆而造成的矮新星，就是此现象的例子。
12.
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。
13.
The Mass and Angular Momentum Loss from the Edge of the Accretion disc and the Evolution of Cataclysmic Binaries
吸积盘边缘的质量和角动量损失与激变双星的演化
14.
Amplification of Magnetic Field in Accretion Disk and Transition of Spectral States in Black Hole Binaries
黑洞吸积盘中磁场的放大及黑洞双星的谱态转变
15.
The model comprising accretion onto a neutron star or black hole companion must still be considered a favored hypothesis.
在中子星或黑洞伴星上发生吸积的模型，仍应看成是一个有价值的假说。
16.
fan for extracting by suction, dus,t steam, smoke, hot gases,etc. whether or not fitted with an integral motor
用于抽吸灰尘、蒸汽、烟、热气等的风扇,无论是是否装有积分电机
17.
Relating to, caused by, or carried by the wind.
风的，风成的或风积的
18.
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。