Properties of Barred Galaxies with the Environment: II. The case of the Cosmic Web around the Virgo cluster

Abstract

Context. Bars are elongated structures developed by a large fraction of disk galaxies in their central few kiloparsecs. However, the bar formation process is still not fully understood, particularly the role played by the galaxy environment in the formation and evolution of these structures. Aims. The aim of this work is to establish how the galaxy environment affects the evolution of bars by analyzing the bar structural parameters in a sample of galaxies located in three different galaxy environments: in the Virgo cluster, in filaments in the Cosmic Web around it, and in the field. Methods. We performed structural analysis using optical imaging from the DESI Legacy survey, measuring bar radii and disk scale lengths through Fourier analysis and surface brightness fitting techniques. Results. After defining a homogeneous sample of barred galaxies across the three different galaxy environments in terms of color and magnitude, the median bar radii were found to be 2.54 +/- 0.34 kpc, 3.29 +/- 0.38 kpc, and 4.44 +/- 0.81 kpc in the cluster, filaments, and field environments, respectively. In addition, the median bar radii scaled by the disk scale lengths was found to be 1.26 +/- 0.09, 1.72 +/- 0.11, and 2.57 +/- 0.21 in the cluster, filaments, and field environments, respectively. These results indicate that the galaxy environment has a significant influence on the structural parameters of bars, with bars in high-density environments being shorter and less prominent than those in the field. Conclusions. Our findings can be interpreted in terms of a slowing of the secular evolution of bars in dense galaxy environments. Barred galaxies located in clusters could experience a reduced rate of bar secular evolution due to various physical processes that occur in high-density environments, such as gas stripping, strangulation, or tidal interactions.

Accepted for publication in A&A

References in corpus (23)

• Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
• The Cosmic Evolution Survey (COSMOS) -- Overview
• Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
• HyperLEDA. III. The catalogue of extragalactic distances
• The Structure of the Milky Way's Bar Outside the Bulge
• The population of barred galaxies in the local universe I. Detection and characterisation of bars
• CALIFA: a diameter-selected sample for an integral field spectroscopy galaxy survey
• LoCuSS: The slow quenching of star formation in cluster galaxies and the need for pre-processing
• Properties of Bars and Bulges in the Hubble Sequence
• The Role of Environment in the Mass-Metallicity Relation
• Quantifying the role of bars in the build-up of central mass concentrations in disk galaxies
• On the Origin of Dwarf Elliptical Galaxies: The Fundamental Plane
• Galaxy Zoo: Are Bars Responsible for the Feeding of Active Galactic Nuclei at 0.2 < z < 1.0?
• A numerical study of interactions and stellar bars
• Frequency and properties of bars in cluster and field galaxies at intermediate redshifts
• Bars and spirals in tidal interactions with an ensemble of galaxy mass models
• The environment of barred galaxies in the low-redshift Universe
• Bars formed in galaxy merging and their classification with deep learning
• Bar-like galaxies in IllustrisTNG
• Observational evidence for bar formation in disk galaxies via cluster-cluster interaction
• Properties of Galaxies in Cosmic Filaments around the Virgo Cluster
• Evidence of a fast bar in the weakly-interacting galaxy NGC 4264 with MUSE
• The Effect of Environment on Galaxy Spiral Arms, Bars, Concentration, and Quenching