The Investigation of the Luminosity Function for Sample 6168 Galaxy Clusters
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Дата
2018
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Анотація
The issue of construction of the luminosity function is an important problem
for analysis of large scale structure statistics and interpretation of astronomical
object counts In the present paper we discuss the the issure of the construction
of the luminosity function for galaxy clusters. The problem is solved based on
counting brightness of galaxies belonging to 6168 galaxy clusters selected from
Panko & Flin (2006) Catalogue. We show that the galaxy clusters are characterized
by the luminosity function signi cantly di erent than that obtained for
both: individual optical galaxies and radiogalaxies. We discuss the signi cance
of this result for the theories of the structure formation.
Опис
Ключові слова
Investigation, Luminosity Function, Sample 6168, Galaxy Clusters
Бібліографічний опис
PTA Proceedings