scholarly journals The Influence of the Peculiar Velocities of SNe Ia in Clusters of Galaxies on the Redshift Measurements

2021 ◽  
Vol 65 (10) ◽  
pp. 897-901
Author(s):  
E. A. Balakina ◽  
M. V. Pruzhinskaya
1987 ◽  
Vol 124 ◽  
pp. 335-348
Author(s):  
Neta A. Bahcall

The evidence for the existence of very large scale structures, ∼ 100h−1Mpc in size, as derived from the spatial distribution of clusters of galaxies is summarized. Detection of a ∼ 2000 kms−1 elongation in the redshift direction in the distribution of the clusters is also described. Possible causes of the effect are peculiar velocities of clusters on scales of 10–100h−1Mpc and geometrical elongation of superclusters. If the effect is entirely due to the peculiar velocities of clusters, then superclusters have masses of order 1016.5M⊙ and may contain a larger amount of dark matter than previously anticipated.


2009 ◽  
Vol 691 (2) ◽  
pp. 1479-1493 ◽  
Author(s):  
A. Kashlinsky ◽  
F. Atrio-Barandela ◽  
D. Kocevski ◽  
H. Ebeling

2021 ◽  
pp. 105-110
Author(s):  
F. G. KOPYLOVA ◽  
A .I. KOPYLOV

We present results of the study of peculiar motions of 57 clusters and groups of galaxies in the regions of the Corona Borealis (CrB), Bootes (Boo), Z 5029/A 1424, A 1190, A 1750/A 1809 superclusters of galaxies and 20 galaxy clusters located beyond massive structures (0.05 z 0.10). Using the SDSS Data Release 8 data, a sample of early-type galaxies was compiled in the systems under study, their Fundamental Planes (FP) were built and relative distances and peculiar velocities were determined.


2008 ◽  
Vol 686 (2) ◽  
pp. L49-L52 ◽  
Author(s):  
A. Kashlinsky ◽  
F. Atrio-Barandela ◽  
D. Kocevski ◽  
H. Ebeling

2012 ◽  
Author(s):  
F. Atrio-Barandela ◽  
A. Kashlinsky ◽  
H. Ebeling ◽  
D. Kocevski ◽  
A. Edge

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