The most recently completed redshift surveys, such as 2dFGRS, reveal spectacularly complex structures in galaxy distribution. These structures are described in terms of filaments, clusters and voids and are usually characterized by using fractal geometry language. In this paper it is shown that the fractal dimension of the large scale distribution of galaxies presents scaling behavior well described by a Verhulst-type law. This result is in agreement with the idea that the Universe we observe today is a self-structured system which emerges from a nonlinear self-organizing phenomenon. Key words: large scale structure, cosmology, structures formation, nonlinear phenomena. 1
This paper discusses if large scale galaxy distribution samples containing almost one million object...
This paper presents a review of the fractal approach for describing the large scale distribution of ...
The fractal structure of star formation on large scales in disk galaxies is studied using the size d...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
In the interstellar medium, as well as in the Universe, large density fluctuations are observed, tha...
A synthesis of the observational data on the distribution of galaxies is made by expressing the stat...
We re-evaluate the experimental data concerning the large scale structure of the universe utilizing ...
We re-evaluate the experimental data concerning the large scale structure of the universe utilizing ...
There is evidence of a scale-invariant matter distribution up to scales over 10 Megaparsecs. We revi...
This paper discusses if large scale galaxy distribution samples containing almost one million object...
This paper presents a review of the fractal approach for describing the large scale distribution of ...
The fractal structure of star formation on large scales in disk galaxies is studied using the size d...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
Past surveys have revealed that the large-scale distribution of galaxies in the universe is far from...
In the interstellar medium, as well as in the Universe, large density fluctuations are observed, tha...
A synthesis of the observational data on the distribution of galaxies is made by expressing the stat...
We re-evaluate the experimental data concerning the large scale structure of the universe utilizing ...
We re-evaluate the experimental data concerning the large scale structure of the universe utilizing ...
There is evidence of a scale-invariant matter distribution up to scales over 10 Megaparsecs. We revi...
This paper discusses if large scale galaxy distribution samples containing almost one million object...
This paper presents a review of the fractal approach for describing the large scale distribution of ...
The fractal structure of star formation on large scales in disk galaxies is studied using the size d...