High-order 3D Voronoi tessellation for identifying isolated galaxies, pairs and triplets |
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Authors: | A Elyiv O Melnyk I Vavilova |
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Institution: | Main Astronomical Observatory, Academy of Sciences of Ukraine, 27 Akademika Zabolotnoho St., 03680 Kyiv, Ukraine;Astronomical Observatory, Kyiv National University, 3 Observatorna St., 04053 Kyiv, Ukraine;Space Research Institute, National Space Agency of Ukraine, National Academy of Sciences of Ukraine, 40 Akdemika Glushkova av., 03680 Kyiv, Ukraine |
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Abstract: | A geometric method based on the high-order 3D Voronoi tessellation is proposed for identifying single galaxies, pairs and triplets. This approach allows us to select small galaxy groups and isolated galaxies in different environments and to find the isolated systems. The volume-limited sample of galaxies from the Sloan Digital Sky Survey Data Release 5 spectroscopic survey was used. We conclude that in such small groups as pairs and triplets, segregation by luminosity is clearly observed: galaxies in isolated pairs and triplets are on average two times more luminous than isolated galaxies. We consider the dark matter content in different systems. The median values of mass-to-luminosity ratio are 12 M⊙/L⊙ for the isolated pairs and 44 M⊙/L⊙ for the isolated triplets, and 7 (8) M⊙/L⊙ for the most compact pairs (triplets). We also found that systems in denser environments have greater rms velocity and mass-to-luminosity ratio. |
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Keywords: | galaxies: general galaxies: kinematics and dynamics dark matter |
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