%0 Journal Article
%T 透镜星系的非距离红移<br>Non-Distance Redshift of Lenticular Galaxies
%A 陈军利
%J Astronomy and Astrophysics
%P 72-85
%@ 2329-1265
%D 2024
%I Hans Publishing
%R 10.12677/aas.2024.124007
%X 本文分析了引力透镜中光线弯曲的康普顿效应&#65292;从而推断出光线弯曲会产生非距离红移&#65292;说明透镜星系的红移大于哈勃红移&#65292;应用红移计算透镜星系中源天体的距离时&#65292;应该减掉透镜星系的非距离红移&#65292;另外&#65292;本文用实例说明了透镜星系中心都存在高亮度星系(星系)&#65292;从而说明了光线弯曲是由可见光从大质量发光星球旁边经过时&#65292;可见光与中心星系发出的电磁波连续作用的结果。<br>This article analyzes the Compton effect of light bending in gravitational lensing, and infers that light bending will produce non-distance redshift, indicating that the redshift of lens galaxies is greater than the Hubble redshift. When applying the redshift to calculate the distance of the source object in the lens galaxy, the non-distance redshift of the lens galaxy should be subtracted. In addition, this article uses examples to illustrate that there are high-brightness galaxies (galaxies) in the centers of lens galaxies, thus illustrating that light bending is the result of the continuous interaction between visible light and electromagnetic waves emitted by the central galaxy when a massively luminous star passes by.
%K 引力透镜&#65292
%K 康普顿效应&#65292
%K 哈勃红移&#65292
%K 星系距离<br>Gravitational Lensing
%K Compton Effect
%K Hubble Redshift
%K Galaxy Distances
%U http://www.hanspub.org/journal/PaperInformation.aspx?PaperID=98967