Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-24T12:35:03.111Z Has data issue: false hasContentIssue false
  • English
  • Français

3-D Voronoi's Tessellation as a Tool for Identifying Galaxy Groups

Published online by Cambridge University Press:  01 August 2006

Olga V. Melnyk ,
Andrii A. Elyiv  and
Iryna B. Vavilova
Olga V. Melnyk
Affiliation:
Astronomical Observatory, National Taras Shevshenko University of Kyiv, 3 Observatorna str., Kyiv, 04053, Ukraine email: [email protected]
Andrii A. Elyiv
Affiliation:
Astronomical Observatory, National Taras Shevshenko University of Kyiv, 3 Observatorna str., Kyiv, 04053, Ukraine email: [email protected]
Iryna B. Vavilova
Affiliation:
Astronomical Observatory, National Taras Shevshenko University of Kyiv, 3 Observatorna str., Kyiv, 04053, Ukraine email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

3-D Voronoi's tessellation method has been applied for identifying groups of galaxies in the structure of the Local Supercluster and evaluation of its properties.

Keywords

Local SuperclusterVoronoi tessellationgalaxy groups
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 223
Copyright
Copyright © International Astronomical Union 2007

References

Kiang, T. 1966, Zeitschrift fur Astrophysik 64, 433.Google Scholar
Makarov, D. I. & Karachentsev, I. D. 2000, ASP Conf. Ser. 209, 40.Google Scholar
Melnyk, O. V., Elyiv, A. A. & Vavilova, I. B. 2006, Kinematika i Fizika Nebesnykh Tel 22, 283.Google Scholar
Vavilova, I. B. & Melnik, O. V. 2005, Mathematics and its Applications 55, 203.Google Scholar