2013MNRAS.428..906C


Query : 2013MNRAS.428..906C

2013MNRAS.428..906C - Mon. Not. R. Astron. Soc., 428, 906-911 (2013/January-1)

Stellar populations in superclusters of galaxies.

COSTA-DUARTE M.V., SODRE L.Jr and DURRET F.

Abstract (from CDS):

A catalogue of superclusters of galaxies is used to investigate the influence of the supercluster environment on galaxy populations, considering galaxies brighter than Mr < -21 + 5logh. Empirical spectral synthesis techniques are applied to obtain the stellar population properties of galaxies which belong to superclusters and representative values of stellar population parameters are attributed to each supercluster. We show that richer superclusters present denser environments and older stellar populations. The galaxy populations of superclusters classified as filaments and pancakes are statistically similar, indicating that the morphology of superclusters does not have a significative influence on the stellar populations. Clusters of galaxies within superclusters are also examined in order to evaluate the influence of the supercluster environment on their galaxy properties. Our results suggest that the environment affects galaxy properties but its influence should operate on scales of groups and clusters, more than on the scale of superclusters.

Abstract Copyright: © 2012 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2012)

Journal keyword(s): galaxies: evolution - galaxies: formation - large-scale structure of Universe

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NAME Sloan Great Wall ? ~ ~           ~ 191 0

Query : 2013MNRAS.428..906C

Basic data :
NAME Sloan Great Wall -- Object of Unknown Nature
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NAME SDSS Great Wall NAME Sloan Great Wall

References (191 between 1850 and 2026) (Total 191)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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