eROSITA clusters dynamical state and their impact on the BCG luminosity
arXiv:2503.21066 · doi:10.1051/0004-6361/202452440
Abstract
The Spectrum Roentgen Gamma/eROSITA first public release contains 12,247 clusters and groups. We use the offset between the Brightest Cluster Galaxy (BCG) and the X--ray peak (D) to classify the cluster dynamical state of 3,946 galaxy clusters and groups. The X--ray peaks come from the eROSITA survey while the BCG positions come from the DECaLS DR10 optical data, which includes the DECam eROSITA Survey optical data. We aim to investigate the evolution of the merger and relaxed cluster distributions with redshift and mass, and their impact on the BCG. We model the distribution of D as the sum of two Rayleigh distributions representing the cluster's relaxed and disturbed populations, and explore their evolution with redshift and mass. To explore the impact of the cluster's dynamical state on the BCG luminosity, we separate the main sample according to the dynamical state. We define clusters as relaxed if D < 0.25, disturbed if D>0.5, and as `diverse' otherwise. We find no evolution of the merging fraction in redshift and mass. We observe that the width of the relaxed distribution to increase with redshift, while the width of the two Rayleigh distributions decreases with mass. The analysis reveals that BCGs in relaxed clusters are brighter than BCGs in both the disturbed and diverse cluster population. The most significant differences are found for high mass clusters at higher redshift. The results suggest that BCGs in low-mass clusters are less centrally bound than those in high-mass systems, irrespective of dynamical state. Over time, BCGs in relaxed clusters progressively align with the potential center. This alignment correlates with their luminosity growth relative to BCGs in dynamically disturbed clusters, underscoring the critical role of the clusters dynamical state in regulating BCG evolution. [Abridged]
10 pages, 6 figures, accepted in A&A
References in corpus (43)
- The Gaia mission
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- The eROSITA X-ray telescope on SRG
- Shocks and cold fronts in galaxy clusters
- Galaxy Clusters Discovered via the Sunyaev-Zel'dovich Effect in the 2500-square-degree SPT-SZ survey
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- The SRG/eROSITA all-sky survey: First X-ray catalogues and data release of the western Galactic hemisphere
- Mass Calibration and Cosmological Analysis of the SPT-SZ Galaxy Cluster Sample Using Velocity Dispersion and X-ray Measurements
- Brightest Cluster Galaxies at the Present Epoch
- The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups
- The DECam Local Volume Exploration Survey: Overview and First Data Release
- Redshifts, Sample Purity, and BCG Positions for the Galaxy Cluster Catalog from the first 720 Square Degrees of the South Pole Telescope Survey
- The SRG/eROSITA all-sky survey: Cosmology constraints from cluster abundances in the western Galactic hemisphere
- Cosmological Constraints from DES Y1 Cluster Abundances and SPT Multi-wavelength data
- The Formation of Massive Cluster Galaxies
- The Three Hundred Project: Dynamical state of galaxy clusters and morphology from multi-wavelength synthetic maps
- The DECam Local Volume Exploration Survey Data Release 2
- The Weak Lensing Radial Acceleration Relation: Constraining Modified Gravity and Cold Dark Matter theories with KiDS-1000
- Cosmological Constraints from Galaxy Clusters and Groups in the eROSITA Final Equatorial Depth Survey
- The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Properties and Scaling Relations of Galaxy Clusters and Groups
- Dynamical state for 964 galaxy clusters from Chandra X-ray images
- A joint SZ-Xray-optical analysis of the dynamical state of 288 massive galaxy clusters
- The Three Hundred Project: quest of clusters of galaxies morphology and dynamical state through Zernike Polynomials
- Dynamical state of galaxy clusters evaluated from X-ray images
- The eROSITA Final Equatorial-Depth Survey (eFEDS): Characterization of Morphological Properties of Galaxy Groups and Clusters
- Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
- Galaxy cluster mergers as triggers for the formation of jellyfish galaxies: case study of the A901/2 system
- Cosmological constraints from abundance, weak-lensing and clustering of galaxy clusters: application to the SDSS
- Dependence of the bright end of galaxy luminosity function on cluster dynamical state
- Simulations of the merging galaxy cluster Abell 2034: what determines the level of separation between gas and dark matter
- The role of baryons in self-interacting dark matter mergers
- Simulations of gas sloshing induced by a newly discovered gas poor substructure in galaxy cluster Abell 1644
- The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
- The dynamical state of Abell 2399: a bullet-like cluster
- Unveiling the internal structure of Hercules supercluster
- The effect of cluster dynamical state on ram-pressure stripping
- Probing Saraswati's heart: evaluating the dynamical state of the massive galaxy cluster A2631 through a comprehensive weak-lensing and dynamical analysis
- Galaxy cluster optical mass proxies from probabilistic memberships
- The effect of dynamical states on galaxy clusters populations. I. Classification of dynamical states
- A major galaxy cluster merger caught by eROSITA: weak lensing mass distribution and kinematic description
- Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
- Clash of Titans: The Impact of Cluster Mergers in the Galaxy Cluster Red Sequence
- Clash of Titans: a MUSE dynamical study of the extreme cluster merger SPT-CL J0307-6225
Cited by in corpus (9)
- Counterpart identification and classification for eRASS1 and characterisation of the AGN content
- Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts
- Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
- Robust AGN and host-galaxy decomposition in optical spectral fitting
- DELVE Milky Way Satellite Galaxy Census I: Satellite Population and Survey Selection Function in DES, DELVE, and Pan-STARRS
- DELVE-ing into the Milky Way's Globular Clusters: Assessing extra-tidal features in NGC 5897, NGC 7492, and testing detectability with deeper photometry
- The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering 5 virial radii around NGC 1399 with galaxy properties
- A Value-added Physical Properties Catalog for Low-redshift Galaxies from DESI Legacy Imaging Surveys DR10
- The Limits of Photometric Dynamics: Benchmarking Cluster Relaxation Diagnostics