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Игорь Брылёв 2025-05-09 15:38:57 +03:00
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@ -98,7 +98,7 @@ Astronomers often use the term "flat disk clusters" in this connection. Moreover
![](./media/pic1.47.jpg)
*Figure 1.47. Dimensionality of space on the Planck length scales according to some physicists' ideas[^ref-134]*
However, there are also clusters of the "***regular***" type (the number of galaxies in them ranges from 200 to 11,000)140 , which mainly consist of old ***elliptical*** galaxies containing old stars of the first generation. They also differ from *irregulars in* that they are predominantly *spherical in shape with a strong concentration of galaxies toward the center*, where the density is sometimes 40,000 times higher than the average density of the distribution of galaxies in the Metagalaxy141. If we take elliptical galaxies as a "cosmic" component of this world, and spiral galaxies as a living one, then clusters of the "correct" three-dimensional type inside the "neural network" of "living" elliptical galaxies can be perceived as some nodes of obliquity inside the "network of life".
However, there are also clusters of the "***regular***" type (the number of galaxies in them ranges from 200 to 11,000)[^ref-140] , which mainly consist of old ***elliptical*** galaxies containing old stars of the first generation. They also differ from *irregulars in* that they are predominantly *spherical in shape with a strong concentration of galaxies toward the center*, where the density is sometimes 40,000 times higher than the average density of the distribution of galaxies in the Metagalaxy [^ref-141]. If we take elliptical galaxies as a "cosmic" component of this world, and spiral galaxies as a living one, then clusters of the "correct" three-dimensional type inside the "neural network" of "living" elliptical galaxies can be perceived as some nodes of obliquity inside the "network of life".
So, if we talk about the STRUCTURE of our present Universe (and not consider the remnants of the structure of the Universe when it was very young and had an age of the size of the types of structures of the Universe:
@ -156,3 +156,5 @@ In the next chapter, we take only the first step in this direction.
[^ref-137]: Large-scale structure of the Universe. / *Edited by M. Longyear and J. Einasto.* M.: Mir, 1981\. С. 277\.
[^ref-138]: *Vorontsov-Vel'yaminov B. A.* Extragalactic Astronomy. M.: Nauka, 1978\. С. 407\.
[^ref-139]: *Vorontsov-Vel'yaminov B. A.* Extragalactic Astronomy. M.: Nauka, 1978\. С. 271-272.
[^ref-140]: *Aghekyan T. A.* Stars, Galaxies, Metagalaxy. M.: Nauka, 1981\. С. 216\.
[^ref-141]: *Aghekyan T. A.* Stars, Galaxies, Metagalaxy. M.: Nauka, 1981\. С. 213, 215\.