| 1. | From the extent of the red shifts the recession velocities can be computed .
从红移量可以计算退行速度。 |
| 2. | In chap. 19 we saw that red shifts in stellar spectra result from motions away from the earth .
在第十九章我们已了解到，恒星光谱中的红移是恒星背离地球的运动造成的。 |
| 3. | The redshift means that the quasars are very far away, more distant than the most distant galaxies we can see .
红移意味着类星体是非常非常遥远的天体，比我们观测到的最遥远的星体还要远。 |
| 4. | Owing to the expansion of the universe, an observer today would expect to find these remnants to have undergone a red shift to long wave lengths .
由于宇宙的膨胀，今天的观察者可望找到这些向长波红移了的残余物。 |
| 5. | We measure the redshift by the following parameter ,
我们通常用z来表示红移的幅度： |
| 6. | Linear redshift distortion in galaxy survey
星系巡天中的线性红移畸变效应 |
| 7. | Titanium oxide modified by plasma and red - shift of its response spectrum
2及其响应光谱红移 |
| 8. | The cosmological redshift is not a normal doppler shift
宇宙学的红移并不是平常的都卜勒偏移。 |
| 9. | The greater the amount of redshift , the more rapid the movement
红移的量越多，移动的速度越快。 |
| 10. | Astronomers say that the galactic light has been redshifted
于是天文学家就说星系的光红移了。 |
