diff --git a/src/14_s_factors_coefficients_of_scale_symmetry.md b/src/14_s_factors_coefficients_of_scale_symmetry.md index 0c4cfa2..f343996 100644 --- a/src/14_s_factors_coefficients_of_scale_symmetry.md +++ b/src/14_s_factors_coefficients_of_scale_symmetry.md @@ -88,8 +88,8 @@ At first, astronomers believed that they form something like ***foam*** or ***ho If this is true, then we can say that on mega-scales of \\(10^{27}\\)...\\(10^{28}\\) cm the world is dominated by ***one-dimensional*** structures, since the ratio of the length of these "superwires" to their diameter is 6:1 on average. - -Figure 1.46. "Up close" the cellular structure of the Metagalaxy may be as it is depicted in the drawing by Anya Abrikosova, a school friend of the author's daughter. This purely abstract fantasy "from nothing to do" could also be not accidental +![](./media/pic1.46.jpg) +*Figure 1.46. "Up close" the cellular structure of the Metagalaxy may be as it is depicted in the drawing by Anya Abrikosova, a school friend of the author's daughter. This purely abstract fantasy "from nothing to do" could also be not accidental* Let us now go deeper, to scales of \\(10^{25}\\)- \\(10^{26}\\) cm. Here we enter the world of galaxy clusters and groups[^ref-138]. These are the ones that make up the filaments of super scatterings. The shape of clusters (\~\\(10^{25}\\) cm) and groups (\~\\(10^{24}\\) cm) is predominantly two-dimensional \- they are mostly flat. diff --git a/src/media/pic1.46.jpg b/src/media/pic1.46.jpg new file mode 100644 index 0000000..492c298 Binary files /dev/null and b/src/media/pic1.46.jpg differ diff --git a/src/media/pic1.47.jpg b/src/media/pic1.47.jpg new file mode 100644 index 0000000..a0f4b60 Binary files /dev/null and b/src/media/pic1.47.jpg differ