1.
These elements become part of the interstellar gas and dust.
这些元素成了星际气体和星际尘埃的一部分。
2.
We will be interested in the heat capacity of interstellar gases.
我们感兴趣的是星际气体的热容量。
3.
The magnetic lines of force are in effect glued to the interstellar gas, and they follow the clouds in their capricious motions.
磁力线实际上是紧附在星际气体上，并跟随星际云一道作着变化莫测的运动。
4.
These tiny regions may be condensations in the interstellar gas where stars and planetary systems could be forming.
这些很小的区域可能是能够形成恒星或行星系统的星际气体中的一些凝聚体。
5.
Interstellar gas clouds frequently collide and convert their kinetic energy into shock waves and radiation.
星际气体云经常在碰撞间将动能传给冲击波和辐射。
6.
The concentrations of interstellar gas can now be mapped with much great accuracy than would ever be possible using visible light.
如今，可以画出比用可见光更精确的星际气体聚集图。
7.
The contraction of a cool interstellar gas cloud can proceed in a variety of ways.
一个冷的星际气体云的收缩，可以通过许多不同的方式来进行。
8.
Our assertion that the interstellar gas is definitely no vacuum would seem all the more paradoxical!
我们坚持星际气体决非真空的主张看来愈发荒谬可笑了！
9.
The remnant nebular gas pervades the interplanetary space.
星云的残余气体充斥星际空间。
10.
clouds of particles or gases occurring throughout interstellar space.
遍及星际空间的微粒或气体组成的云。
11.
Such tumultuous, often visually spectacular, interstellar regions surrounding youthful stars are known as gaseous nebulae.
这种环绕着年轻星的动荡且常常是壮观的星际区域，叫做气体星云。
12.
A star is formed when a cloud of gas collapses from the interstellar medium toward high density.
一个气体云自星际物质中坍缩，密度达到很高时，即形成了一个恒星。
13.
International Satellite Cloud Climatology Project
国际卫星云气候学项目
14.
International Satellite Cloud Climatology Project (ISCCP)
国际卫星云气候学计划
15.
International Polar Orbiting Meteorological Satellite
国际极轨道气象卫星
16.
The solar wind does not impinge directly on the earth and its atmosphere, however.
太阳风一直向外吹，直到碰到星际中的离子或电中性气体。
17.
an immense cloud of gas (mainly hydrogen) and dust in interstellar space.
在星际空间中的一种无边的由气体（主要成分为氢）和灰尘组成的云。
18.
We consider the macroscopic thermal properties of the gas throughout the interstellas region ionized by an exciting star or group of stars.
我们将考察被一颗或一群激发星电离的星际区域中各种气体的宏观热力学性质。