# Investigation of properties of galaxy clusters in the Hercules supercluster region

@article{Kopylova2013InvestigationOP,
title={Investigation of properties of galaxy clusters in the Hercules supercluster region},
author={Flera G. Kopylova and Alexander I. Kopylov},
journal={Astronomy Letters},
year={2013},
volume={39},
pages={1-16}
}
• Published 24 January 2013
• Physics
• Astronomy Letters
We investigated the properties of galaxy clusters in the region of the Hercules supercluster using observational data from the SDSS and 2MASS catalogs and the NED. We have selected 13 galaxy clusters with a total dynamical mass of 4.82 × 1015M⊙ in a 100 × 45 Mpc supercluster region in the plane of the sky (0.030 < z < 0.041). In addition, our sample includes eight clusters from the immediate neighborhoods of the superclusters and ten field clusters at the same z. The derived properties of the…
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## References

SHOWING 1-10 OF 34 REFERENCES
Analysis of the properties of galaxy clusters in the Leo supercluster region
• Physics
• 2011
We analyze the properties of galaxy clusters in the region of the Leo supercluster using observational data from the SDSS and 2MASS catalogs. We have selected 14 galaxy clusters with a total
Analysis of the properties of clusters of galaxies in the region of the Ursa Major supercluster
• Physics
• 2009
We analyze the properties of the clusters of galaxies in the region of the Ursa Major (UMa) supercluster using observational data from SDSS and 2MASS catalogs. The region studied includes a
Toward Understanding Rich Superclusters
We present a morphological study of the two richest superclusters from the 2dF Galaxy Redshift Survey (SCL126, the Sloan Great Wall, and SCL9, the Sculptor supercluster). We use Minkowski
Mass Profile of the Infall Region of the Abell 2199 Supercluster
• Physics
• 2002
Using a redshift survey of 1323 galaxies (1092 new or remeasured) in a region of 95 deg2 centered on the nearby galaxy cluster Abell 2199, we analyze the supercluster containing A2199, A2197, and an
K-band Properties of Galaxy Clusters and Groups: Brightest Cluster Galaxies and Intracluster Light
• Physics
• 2004
We investigate the near-infrared K-band properties of the brightest cluster galaxies (BCGs) in a sample of 93 X-ray galaxy clusters and groups, using data from the Two Micron All Sky Survey. Our
Kinematics of the Hercules Supercluster
• Physics
• 1997
?????The Hercules supercluster consists of the Abell clusters A2147, A2151, and A2152. Previous studies of the kinematics have been confounded by the difficulty of correctly assigning galaxies to the
SDSS DR7 superclusters - Morphology
Aims. We study the morphology of a set of superclusters drawn from the SDSS DR7. Methods. We calculate the luminosity density field to determine super clusters from a flux-limited sample of galaxies
K-Band Properties of Galaxy Clusters and Groups: Luminosity Function, Radial Distribution, and Halo Occupation Number
• Physics
• 2004
We explore the near-infrared (NIR) K-band properties of galaxies within 93 galaxy clusters and groups using data from the Two Micron All Sky Survey. We use X-ray properties of these clusters to
CAIRNS: The Cluster and Infall Region Nearby Survey. II. Environmental Dependence of Infrared Mass-to-Light Ratios
• Physics
• 2004
CAIRNS (Cluster and Infall Region Nearby Survey) is a spectroscopic survey of the infall regions surrounding nine nearby rich clusters of galaxies. In our previous paper, we used redshifts within ~10
K-Band Properties of Well-Sampled Groups of Galaxies
• Physics
• 2004
We use a sample of 55 groups and six clusters of galaxies ranging in mass from 7 × 1011 to 1.5 × 1015 M⊙ to examine the correlation of the Ks-band luminosity with mass discovered by Lin and coauthors