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Clusters and Voids in General Galaxy Field
Symposium - International Astronomical Union, 1996In our previous works (Anosova 1987, Anosova, Iyer, Varma 1994), we developed a new method for determination of the structure of a clustered distribution. In this work, we apply this method studying the observed distribution of galaxies in the Universe.
J. Anosova, S. Iyer, R. K. Varma
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Vortex Generation by Shock-Bubble Interaction in Galaxy Clusters
2015Fluid mechanics is at the heart of almost all astronomical research. In many cases, the conditions in astrophysical systems are such that supersonic flows are common. As a result, the most energetic phenomena in astronomy all involve some form of shock physics, often relativistic.
S. Heinz, S. Friedman, E. Churazov
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Next-Generation Images of Galaxy Clusters at Millimeter Wavelengths
Galaxy clusters are the largest and most massive objects in the universe. Observing and studying them unlocks answers to broad cosmological questions, such as the matter content and its distribution in the universe, as well as more specific astrophysical topics regarding the nature of physics within the intracluster medium (ICM).openaire +2 more sources
Galaxies' clustering generalized theory DARK-D-21-00019R2
2021M Hameeda, Plastino, Angelo, M C Rocca
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