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- W4309209462 abstract "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 semi-automatic analysis of ellipticity and position angle profiles. We find, in agreement with previous studies, a strong co-dependence 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." @default.
- W4309209462 created "2022-11-24" @default.
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- W4309209462 date "2022-11-01" @default.
- W4309209462 modified "2023-10-15" @default.
- W4309209462 title "Morphology Driven Evolution of Barred Galaxies in OMEGAWINGS Clusters" @default.
- W4309209462 cites W1893350802 @default.
- W4309209462 cites W1934193987 @default.
- W4309209462 cites W1946092078 @default.
- W4309209462 cites W1973416141 @default.
- W4309209462 cites W1975150389 @default.
- W4309209462 cites W1982051859 @default.
- W4309209462 cites W2001678324 @default.
- W4309209462 cites W2003092390 @default.
- W4309209462 cites W2004701242 @default.
- W4309209462 cites W2006796627 @default.
- W4309209462 cites W2009330294 @default.
- W4309209462 cites W2021256493 @default.
- W4309209462 cites W2031521127 @default.
- W4309209462 cites W2032881850 @default.
- W4309209462 cites W2034085752 @default.
- W4309209462 cites W2048502077 @default.
- W4309209462 cites W2051842911 @default.
- W4309209462 cites W2055327934 @default.
- W4309209462 cites W2055443781 @default.
- W4309209462 cites W2056770290 @default.
- W4309209462 cites W2059588423 @default.
- W4309209462 cites W2064620738 @default.
- W4309209462 cites W2066452342 @default.
- W4309209462 cites W2069360457 @default.
- W4309209462 cites W2090887265 @default.
- W4309209462 cites W2120880319 @default.
- W4309209462 cites W2121729638 @default.
- W4309209462 cites W2123132830 @default.
- W4309209462 cites W2129802004 @default.
- W4309209462 cites W2130527528 @default.
- W4309209462 cites W2133436825 @default.
- W4309209462 cites W2136651428 @default.
- W4309209462 cites W2139445185 @default.
- W4309209462 cites W2156074389 @default.
- W4309209462 cites W2157064517 @default.
- W4309209462 cites W2164297197 @default.
- W4309209462 cites W2168113537 @default.
- W4309209462 cites W2168297159 @default.
- W4309209462 cites W2168500673 @default.
- W4309209462 cites W2401786960 @default.
- W4309209462 cites W2490854898 @default.
- W4309209462 cites W2730569400 @default.
- W4309209462 cites W2768553244 @default.
- W4309209462 cites W2783040051 @default.
- W4309209462 cites W2794539767 @default.
- W4309209462 cites W2801880648 @default.
- W4309209462 cites W2897644201 @default.
- W4309209462 cites W2993807219 @default.
- W4309209462 cites W3023871854 @default.
- W4309209462 cites W3025636298 @default.
- W4309209462 cites W3082470640 @default.
- W4309209462 cites W3086893339 @default.
- W4309209462 cites W3089235226 @default.
- W4309209462 cites W3090987257 @default.
- W4309209462 cites W3091810622 @default.
- W4309209462 cites W3098207073 @default.
- W4309209462 cites W3098525581 @default.
- W4309209462 cites W3098765963 @default.
- W4309209462 cites W3098779512 @default.
- W4309209462 cites W3099072353 @default.
- W4309209462 cites W3099141152 @default.
- W4309209462 cites W3100024326 @default.
- W4309209462 cites W3100220540 @default.
- W4309209462 cites W3100222814 @default.
- W4309209462 cites W3100562678 @default.
- W4309209462 cites W3102402854 @default.
- W4309209462 cites W3102729199 @default.
- W4309209462 cites W3102804177 @default.
- W4309209462 cites W3103233148 @default.
- W4309209462 cites W3103282987 @default.
- W4309209462 cites W3103502977 @default.
- W4309209462 cites W3103877238 @default.
- W4309209462 cites W3104349085 @default.
- W4309209462 cites W3104822455 @default.
- W4309209462 cites W3105933126 @default.
- W4309209462 cites W3106487884 @default.
- W4309209462 cites W3121770305 @default.
- W4309209462 cites W3124615622 @default.
- W4309209462 cites W4248987285 @default.
- W4309209462 cites W4292310804 @default.
- W4309209462 cites W4298349320 @default.
- W4309209462 doi "https://doi.org/10.3847/1538-4357/ac9976" @default.
- W4309209462 hasPublicationYear "2022" @default.
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