inner accretion flow 内吸积流
hot accretion flow 热吸积流
accretion n flow 吸积流
channel-flow accretion 渠道流量增长
channel flow accretion 河槽水流增加
In the first half of this paper, namely the 1st and 2rd chapter, a summary review are presented for the history of accretion theory and an new important theoretical branch, radiatively inefficient accretion flow (RIAF).
本文的前半部分即第一、二两章,主要是简单回顾了吸积理论的发展历史和对吸积理论的一个新的重要分支——辐射冷却无效吸积流——做了一个简略的综述。
参考来源 - 物质外流对辐射冷却无效吸积流的影响·2,447,543篇论文数据，部分数据来源于NoteExpress
These results agree with the major features of the accretion flow by the magnetic neutron star.
这些结果与中子星吸积流动的主要特征一致。
We investigate the linear stability of a shocked accretion flow onto a black hole with the following procedures: First, we study the stability in the inviscid isothermal limit.
我们按如下步骤研究了含激波的黑洞吸积流的线性稳定性问题：首先，我们研究无粘滞的等温吸积流。
For a stationary, adiabatic flow the specific energy E, specific angular momentum L and mass accretion rate M are constant in space.
对于静态、绝热吸积流，比能量E、比角动量L和质量吸积率M都是空间的常量。
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