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- W4294958422 abstract "We study the impact of local environment on the transformation of spiral galaxies in three nearby ($z < 0.08$) Abell clusters: A85/A496/A2670. These systems were observed in HI with the Very Large Array, covering a volume extending beyond the virial radius and detecting 10, 58, 38 galaxies, respectively. High fractions (0.40--0.86) of bright spirals [log$(M_{*}/M_{odot})=9-10$] are not detected in HI. We provide further evidence of environmental effects consisting in significant fractions (0.10--0.33) of abnormal objects and a number of red (passive) spirals, suggesting an ongoing process of quenching. Ram-pressure profiles, and the sample of the brightest spirals used as test particles for environmental effects, indicate that ram-pressure plays an important role in stripping and transforming late-types. Phase-space diagrams and our search for substructures helped to trace the dynamical stage of the three systems. This was used to compare the global cluster effects $vs.$ pre-processing, finding that the former is the dominating mechanism in the studied clusters. By contrasting the global distribution of HI normal $vs.$ HI disturbed spirals in the combined three clusters, we confirm the expected correlation of disturbed objects located, on average, at shorter projected radii. However, individual clusters do not necessarily follow this trend and we show that A496 and A2670 present an atypical behavior. In general we provide conclusive evidence about the dependence of the transformation of infalling spirals on the ensemble of cluster properties like mass, ICM density, dynamical stage and surrounding large-scale structure." @default.
- W4294958422 created "2022-09-08" @default.
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- W4294958422 date "2022-09-08" @default.
- W4294958422 modified "2023-10-01" @default.
- W4294958422 title "Environmental cluster effects and galaxy evolution: The H <scp>i</scp> properties of the Abell clusters A85/A496/A2670" @default.
- W4294958422 cites W1603209501 @default.
- W4294958422 cites W1609444141 @default.
- W4294958422 cites W1613735089 @default.
- W4294958422 cites W1869308734 @default.
- W4294958422 cites W1966928945 @default.
- W4294958422 cites W1973086803 @default.
- W4294958422 cites W1973416141 @default.
- W4294958422 cites W1974132587 @default.
- W4294958422 cites W1974144053 @default.
- W4294958422 cites W1977637580 @default.
- W4294958422 cites W1981427545 @default.
- W4294958422 cites W1983063361 @default.
- W4294958422 cites W1994483112 @default.
- W4294958422 cites W1995641972 @default.
- W4294958422 cites W1997201902 @default.
- W4294958422 cites W1999127286 @default.
- W4294958422 cites W2002569490 @default.
- W4294958422 cites W2007325934 @default.
- W4294958422 cites W2013497789 @default.
- W4294958422 cites W2019126899 @default.
- W4294958422 cites W2028013311 @default.
- W4294958422 cites W2031521127 @default.
- W4294958422 cites W2033510106 @default.
- W4294958422 cites W2033654844 @default.
- W4294958422 cites W2041335483 @default.
- W4294958422 cites W2044548694 @default.
- W4294958422 cites W2046620005 @default.
- W4294958422 cites W2047170523 @default.
- W4294958422 cites W2048758550 @default.
- W4294958422 cites W2051870974 @default.
- W4294958422 cites W2055327934 @default.
- W4294958422 cites W2059594277 @default.
- W4294958422 cites W2060439377 @default.
- W4294958422 cites W2060673519 @default.
- W4294958422 cites W2064056132 @default.
- W4294958422 cites W2073008730 @default.
- W4294958422 cites W2074106980 @default.
- W4294958422 cites W2077334492 @default.
- W4294958422 cites W2084775077 @default.
- W4294958422 cites W2088881638 @default.
- W4294958422 cites W2092640027 @default.
- W4294958422 cites W2117537060 @default.
- W4294958422 cites W2123482074 @default.
- W4294958422 cites W2139445185 @default.
- W4294958422 cites W2155416414 @default.
- W4294958422 cites W2158452591 @default.
- W4294958422 cites W2162290847 @default.
- W4294958422 cites W2165003596 @default.
- W4294958422 cites W2173961484 @default.
- W4294958422 cites W2342588813 @default.
- W4294958422 cites W2603174278 @default.
- W4294958422 cites W2609931621 @default.
- W4294958422 cites W2759542770 @default.
- W4294958422 cites W2773188155 @default.
- W4294958422 cites W2782802313 @default.
- W4294958422 cites W2788475275 @default.
- W4294958422 cites W2792981659 @default.
- W4294958422 cites W2804099527 @default.
- W4294958422 cites W2806883577 @default.
- W4294958422 cites W2807149963 @default.
- W4294958422 cites W2891989599 @default.
- W4294958422 cites W2903093030 @default.
- W4294958422 cites W2911171117 @default.
- W4294958422 cites W2911180026 @default.
- W4294958422 cites W2993807219 @default.
- W4294958422 cites W3007336023 @default.
- W4294958422 cites W3012981346 @default.
- W4294958422 cites W3022142054 @default.
- W4294958422 cites W3034196615 @default.
- W4294958422 cites W3046893667 @default.
- W4294958422 cites W3094818009 @default.
- W4294958422 cites W3098454738 @default.
- W4294958422 cites W3098719395 @default.
- W4294958422 cites W3098843396 @default.
- W4294958422 cites W3099938284 @default.
- W4294958422 cites W3099957511 @default.
- W4294958422 cites W3100095145 @default.
- W4294958422 cites W3101440654 @default.
- W4294958422 cites W3102062140 @default.
- W4294958422 cites W3103493368 @default.
- W4294958422 cites W3103737884 @default.
- W4294958422 cites W3104519067 @default.
- W4294958422 cites W3104843703 @default.
- W4294958422 cites W3105009439 @default.