10 citations · 29 across the 19 of their papers we have counts for
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Continuous Filament Network of the Local Universe
Anatoliy Tugay, Mariusz Tarnopolski
Simulated galaxy distributions are suitable for developing filament detection algorithms. However, samples of observed galaxies, being of limited size, cause difficulties that lead…
X-ray Emission and Orientation of Selected PF Galaxy Clusters
A. V. Tugay, S. S. Dylda, E. A. Panko
X-ray counterparts for 35 galaxy clusters contained in the PF catalog of galaxy clusters and groups were found in XMM-Newton archive. 22 ones (all from ACO catalogue) have extended…
Statistical Analysis of Large-Scale Structure of Universe
A. V. Tugay
While galaxy cluster catalogs were compiled many decades ago, other structural elements of cosmic web are detected at definite level only in the newest works. For example, extragal…
Determination of the Galaxy Cluster Orientation Using X-ray Images by FOCAS Method
A. V. Tugay, S. Yu. Shevchenko
In our work we considered orientations of bright X-ray halos of the galaxy clusters (mainly Abell clusters). 78 appropriate clusters were selected using data from Xgal sample of ex…
Simulation of Large-Scale Structure of Universe by Gaussian Random Fields
V. V. Voitsekhovskiy, A. V. Tugay
Large-scale structure of Universe includes galaxy clusters connected by filaments. Voids occupy the rest of cosmic volume. The search of any dependencities in filament structure ca…
Numerical Estimator for Large-Scale Cosmic Structures
A. V. Tugay, N. G. Pulatova, A. D. Zhoga
Components of large-scale structure (LSS) of Universe includes galaxy clusters, walls, filaments, groups and field galaxies. The question of spatial organization of all these compo…