Hostname: page-component-84b7d79bbc-fnpn6 Total loading time: 0 Render date: 2024-07-29T18:00:08.981Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  01 August 2006

Olga V. Melnyk
Affiliation:
Astronomical Observatory, National Taras Shevshenko University of Kyiv, 3 Observatorna str., Kyiv, 04053, Ukraine email: melnykov@observ.univ.kiev.ua
Andrii A. Elyiv
Affiliation:
Astronomical Observatory, National Taras Shevshenko University of Kyiv, 3 Observatorna str., Kyiv, 04053, Ukraine email: melnykov@observ.univ.kiev.ua
Iryna B. Vavilova
Affiliation:
Astronomical Observatory, National Taras Shevshenko University of Kyiv, 3 Observatorna str., Kyiv, 04053, Ukraine email: melnykov@observ.univ.kiev.ua
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.

Type
Contributed Papers
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