Fundamental Plane of Groups and Clusters of Galaxies: Distances and Peculiar Velocities of Superclusters of Galaxies on Small Scales
Flera G. Kopylova, Alexander I Kopylov

TL;DR
This study extends the fundamental plane of galaxy groups and clusters, enabling distance measurement and first-time peculiar velocity estimation of superclusters, with implications for understanding large-scale cosmic flows.
Contribution
It presents an expanded sample of galaxy systems, refines the fundamental plane relation, and measures peculiar velocities of superclusters for the first time.
Findings
Fundamental plane relation: $L_K \,\propto\ R_e^{0.77} \sigma^{1.44}$.
Distance error in galaxy systems is approximately 16%.
Mean peculiar velocity of superclusters is $+75\pm360$ km/s.
Abstract
This work is a continuation of the work of Kopylova and Kopylov (2016) to build a fundamental plane (FP) of groups and clusters of galaxies -- here a sample of galaxies systems is increased from 94 to 172 objects. We have studied the ratios between the basic characteristics of groups and clusters of galaxies according to the archival data of SDSS, 2MASX and NED catalogs. Measured parameters (, and ) of clusters of galaxies determine the fundamental plane in the near infrared region: . The form of the FP of groups/clusters is consistent with the FP of the early -- types of galaxies (SDSS, -band) determined in the same way. Direct regression relative to the padius in the kpc gives a projection of the FP -- $\log R_e=0.98(\pm0.06)\,\log \sigma-0.56(\pm0.04)<\log \langle I_e…
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
TopicsMaterial Science and Thermodynamics · Differential Equations and Numerical Methods · Historical Geography and Cartography
