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• W2019934556 abstract "We study the role of the environment on galaxy evolution using a sample of 868 galaxies in the Virgo cluster and in its surrounding regions that are selected from the GALEX Ultraviolet Virgo Cluster Survey (GUViCS) with the purpose of understanding the origin of the red sequence in dense environments. The sample spans a wide range in morphological types (from dwarf ellipticals to Im and BCD) and stellar masses (10 7 Mstar 10 11.5 M� ). We collected multifrequency data covering the whole electromagnetic spectrum for most of the galaxies, including UV, optical, mid- and far-infrared imaging data, as well as optical and HI spectroscopic data. We first identify the different dynamical substructures that compose the Virgo cluster, and we calculate the local density of galaxies using different methods. We then study the distribution of galaxies belonging to the red sequence, the green valley, and the blue cloud within the different cluster substructures or as a function of galaxy density. Our analysis indicates that all the most massive galaxies (Mstar 10 11 M� ) are slow rotators and are the dominant galaxies of the different cluster substructures, which are generally associated with a diffuse X-ray emission. They are probably the result of major merging events that occurred at early epochs, as also indicated by their very old stellar populations. Slow rotators of lower stellar mass (10 8.5 Mstar 10 11 M� ) are also preferentially located within the different high-density substructures of the cluster. Their position in the velocity space indicates that they are virialised within the cluster; thus, they are Virgo members since its formation. They have been shaped by gravitational perturbations occurring within the infalling groups that later form the cluster (pre-processing). On the contrary, low-mass star-forming systems are extremely rare in the inner regions of the Virgo cluster A, where the density of the intergalactic medium is at its maximum. Our ram pressure stripping models consistently indicate that these star-forming systems can be rapidly deprived of their interstellar medium during their interaction with the intergalactic medium. The lack of gas quenches their star-formation activity transforming them into quiescent dwarf ellipticals. This mild transformation does not perturb the kinematic properties of these galaxies, which still have rotation curves typical of star-forming systems." @default.
• W2019934556 created "2016-06-24" @default.
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• W2019934556 date "2014-10-01" @default.
• W2019934556 modified "2023-10-18" @default.
• W2019934556 title "The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV: The role of the cluster environment on galaxy evolution" @default.
• W2019934556 cites W1491681531 @default.
• W2019934556 cites W1586340492 @default.
• W2019934556 cites W1679225015 @default.
• W2019934556 cites W1827209908 @default.
• W2019934556 cites W1865085185 @default.
• W2019934556 cites W1964344398 @default.
• W2019934556 cites W1973221593 @default.
• W2019934556 cites W1976806349 @default.
• W2019934556 cites W1979424991 @default.
• W2019934556 cites W1980088203 @default.
• W2019934556 cites W1982330764 @default.
• W2019934556 cites W1985386646 @default.
• W2019934556 cites W1985952407 @default.
• W2019934556 cites W1987522415 @default.
• W2019934556 cites W1989782097 @default.
• W2019934556 cites W1990479339 @default.
• W2019934556 cites W1990629543 @default.
• W2019934556 cites W1994145175 @default.
• W2019934556 cites W1998277739 @default.
• W2019934556 cites W2002038882 @default.
• W2019934556 cites W2004330941 @default.
• W2019934556 cites W2006878995 @default.
• W2019934556 cites W2007325934 @default.
• W2019934556 cites W2011029693 @default.
• W2019934556 cites W2013642036 @default.
• W2019934556 cites W2015117109 @default.
• W2019934556 cites W2019783281 @default.
• W2019934556 cites W2020401182 @default.
• W2019934556 cites W2021008553 @default.
• W2019934556 cites W2022245364 @default.
• W2019934556 cites W2024674795 @default.
• W2019934556 cites W2029792579 @default.
• W2019934556 cites W2033654844 @default.
• W2019934556 cites W2034933552 @default.
• W2019934556 cites W2037816278 @default.
• W2019934556 cites W2042765170 @default.
• W2019934556 cites W2046620005 @default.
• W2019934556 cites W2048758550 @default.
• W2019934556 cites W2049658715 @default.
• W2019934556 cites W2052755662 @default.
• W2019934556 cites W2052923345 @default.
• W2019934556 cites W2052937506 @default.
• W2019934556 cites W2054892752 @default.
• W2019934556 cites W2055327934 @default.
• W2019934556 cites W2060448616 @default.
• W2019934556 cites W2062215462 @default.
• W2019934556 cites W2067062904 @default.
• W2019934556 cites W2067342622 @default.
• W2019934556 cites W2071079352 @default.
• W2019934556 cites W2072965718 @default.
• W2019934556 cites W2073915977 @default.
• W2019934556 cites W2075974992 @default.
• W2019934556 cites W2077622335 @default.
• W2019934556 cites W2077677140 @default.
• W2019934556 cites W2080561301 @default.
• W2019934556 cites W2080807393 @default.
• W2019934556 cites W2080931424 @default.
• W2019934556 cites W2082302236 @default.
• W2019934556 cites W2084775077 @default.
• W2019934556 cites W2086573197 @default.
• W2019934556 cites W2088536005 @default.
• W2019934556 cites W2094796460 @default.
• W2019934556 cites W2101436117 @default.
• W2019934556 cites W2102738222 @default.
• W2019934556 cites W2107337450 @default.
• W2019934556 cites W2107779776 @default.
• W2019934556 cites W2109896455 @default.
• W2019934556 cites W2111392735 @default.
• W2019934556 cites W2111817932 @default.
• W2019934556 cites W2111841752 @default.
• W2019934556 cites W2112966748 @default.
• W2019934556 cites W2115602332 @default.
• W2019934556 cites W2116466430 @default.
• W2019934556 cites W2117060658 @default.
• W2019934556 cites W2117415486 @default.
• W2019934556 cites W2121023735 @default.
• W2019934556 cites W2121833666 @default.
• W2019934556 cites W2123724105 @default.
• W2019934556 cites W2124199755 @default.
• W2019934556 cites W2124324031 @default.
• W2019934556 cites W2125399517 @default.
• W2019934556 cites W2128670568 @default.

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