Relative distances and peculiar velicities of 140 groups and clusters of galaxies at low redshifts: the Hubble diagram
Flera G. Kopylova, Alexander I. Kopylov

TL;DR
This study uses the fundamental plane of early-type galaxies to determine relative distances and peculiar velocities of 140 galaxy groups and clusters at low redshifts, constructing a Hubble diagram consistent with the $ m extLambda$CDM model.
Contribution
It provides new measurements of the Hubble constant and peculiar velocities for galaxy systems using SDSS data and the fundamental plane, with detailed analysis of deviations and large-scale motions.
Findings
Hubble constant estimated as 70 ± 2.8 km/s/Mpc.
Root-mean-square peculiar velocity deviations are 714 ± 7 km/s and 600 ± 7 km/s.
No outflow detected from the Giant Void region.
Abstract
To determine the relative distances and peculiar velocities of 140 groups and clusters of galaxies at low redshifts ( < 0.12), we used the fundamental plane (FP) of early-type galaxies (from the Sloan Digital Sky Survey (SDSS) data). We constructed the Hubble diagram for the relative distances of galaxy groups/clusters versus their radial velocities in the cosmic microwave background (CMB) reference frame in the flat cold dark matter (CDM) model (, ~km~s Mpc). We have found that the standard logarithmic deviation for groups and clusters of galaxies on the Hubble diagram (minus peculiar velocities) is ( = 140), which corresponds to a deviation of ~km~s Mpc in the Hubble constant. For a sample of galaxy systems ( = 63), the X-ray luminosity of which is in an interval of (0.151--4)~$\times…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena
