2022ApJ...940....1T

Query : 2022ApJ...940....1T

2022ApJ...940....1T - Astrophys. J., 940, 1-13 (2022/November-3)

Morphology Driven Evolution of Barred Galaxies in OMEGAWINGS Clusters.

TAWFEEK A.A., SODI B.C., FRITZ J., MORETTI A., PEREZ-MILLAN D., GULLIEUSZIK M., POGGIANTI B.M., VULCANI B. and BETTONI D.

Abstract (from CDS):

We present a study of barred galaxies in the cluster environment, exploiting a sample of galaxies drawn from the extended WIde-field Nearby Galaxy-cluster Survey (OmegaWINGS) that covers up to the outer regions of 32 local X-ray selected clusters. Barred galaxies are identified through a semiautomatic analysis of ellipticity and position angle profiles. We find, in agreement with previous studies, a strong codependence of the bar fraction with the galaxy stellar mass and morphological type, being maximum for massive late-type galaxies. The fraction of barred galaxies decreases with increasing cluster mass and with decreasing clustercentric distance, a dependence that vanishes once we control for morphological type, which indicates that the likelihood of a galaxy hosting a bar in the cluster environment is determined by its morphological transformation. At large clustercentric distances, we detect a dependence on the distance to the nearest neighbor galaxy, suggesting that tidal forces with close companions are able to suppress the formation of bars or even destroy them. Barred galaxies in our sample are either early-type, star-forming galaxies located within the virial radii of the clusters or late-type quenched galaxies found beyond the virial radii of the clusters. We propose a scenario in which already quenched barred galaxies that fall into the clusters are centrally rejuvenated by the interplay of the perturbed gas by ram pressure and the bar, in galaxies that are undergoing a morphological transformation.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Galaxy clusters - Galaxy evolution

Simbad objects: 35

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Number of rows : 35
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 ACO 2717 ClG 00 03 12.9 -35 56 13           ~ 146 0
2 ACO 2734 ClG 00 11 21.60 -28 51 16.6           ~ 156 0
3 ACO 85 ClG 00 41 36.21 -09 19 30.4           ~ 974 0
4 ACO 151 ClG 01 08 52.3 -15 25 01           ~ 199 1
5 ACO 168 ClG 01 15 07.58 +00 19 10.8           ~ 379 2
6 ACO 193 ClG 01 25 07.3 +08 41 36           ~ 192 0
7 ACO 3128 ClG 03 29 50.6 -52 34 48           ~ 183 3
8 ACO 3158 ClG 03 43 07.5 -53 38 09           ~ 327 0
9 ACO 3266 ClG 04 31 26.4 -61 25 17           ~ 447 0
10 ACO 500 ClG 04 38 55.0 -22 05 55           ~ 89 0
11 ACO 3367 ClG 05 49 21 -24 28.1           ~ 34 0
12 ACO 3376 ClG 06 01 25.000 -39 59 51.00           ~ 334 0
13 ACO 3395 ClG 06 27 31.1 -54 23 58           ~ 229 0
14 ACO 754 ClG 09 09 14.8 -09 40 35           ~ 695 1
15 ACO 957 ClG 10 14 02.35 -00 53 30.0           ~ 225 2
16 ACO 970 ClG 10 17 34.3 -10 42 01           ~ 93 0
17 NAME Virgo Cluster ClG 12 30 47.8 +12 23 07           ~ 7107 0
18 [FMV2006] A1631a ClG 12 52 52 -15 24.0           ~ 17 0
19 ACO 3528 ClG 12 54 18.2 -29 01 16           ~ 166 1
20 ACO 3530 ClG 12 55 36.0 -30 20 49           ~ 109 0
21 ACO 3532 ClG 12 57 19.2 -30 22 13           ~ 185 2
22 ACO 1656 ClG 12 59 44.40 +27 54 44.9           ~ 5141 2
23 ACO 3556 ClG 13 24 06.2 -31 39 38           ~ 159 0
24 ACO 3558 ClG 13 28 03.2 -31 31 35           ~ 476 2
25 ACO 3560 ClG 13 32 23.7 -33 08 21           ~ 145 1
26 ACO 3667 ClG 20 12 33.68 -56 50 26.3           ~ 676 1
27 ACO 3716 ClG 20 51 16.7 -52 41 43           ~ 123 1
28 Z 375-15 BiC 21 13 55.918 +02 33 55.39   15.1       ~ 67 1
29 ACO 3809 ClG 21 46 57.5 -43 54 06           ~ 99 0
30 ACO 2382 ClG 21 51 57.2984 -15 36 48.067           ~ 122 0
31 ACO 2399 ClG 21 57 19.01 -07 50 57.5           ~ 197 0
32 ACO 2415 ClG 22 05 25.0 -05 35 23           ~ 124 1
33 ACO 3880 ClG 22 27 49.5 -30 34 40           ~ 104 2
34 ACO 2457 ClG 22 35 40.30 +01 31 33.6           ~ 139 0
35 ACO 4059 ClG 23 57 02.2 -34 45 58           ~ 400 1

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