因此，通过对畸变的观测，可以确定富星系团内电子的密度和温度以及哈勃常数h_0。

Hence it is proposed that the temperature and the density of electrons in a rich cluster and the Hubble constant H0 may be determined from the observations of the IR-background distortion.

youdao

因此，通过对畸变的观测，可以确定富星系团内电子的密度和温度以及哈勃常数h_0。

Hence it is proposed that the temperature and the density of electrons in a rich cluster and the Hubble constant H0 may be determined from the observations of the IR-background distortion.

youdao