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- W2097957963 abstract "We investigate the properties of optically passive spirals and dusty red galaxies in the A901/2 cluster complex at redshift ∼0.17 using rest-frame near-ultraviolet–optical spectral energy distributions, 24-μm infrared data and Hubble Space Telescope morphologies from the STAGES data set. The cluster sample is based on COMBO-17 redshifts with an rms precision of σcz ≈ 2000 km s −1 . We find that ‘dusty red galaxies’ and ‘optically passive spirals’ in A901/2 are largely the same phenomenon, and that they form stars at a substantial rate, which is only four times lower than that in blue spirals at fixed mass. This star formation is more obscured than in blue galaxies and its optical signatures are weak. They appear predominantly in the stellar mass range of log M∗/M� = [10, 11] where they constitute over half of the star-forming galaxies in the cluster; they are thus a vital ingredient for understanding the overall picture of star formation quenching in clusters. We find that the mean specific star formation rate (SFR) of star-forming galaxies in the cluster is clearly lower than in the field, in contrast to the specific SFR properties of blue galaxies alone, which appear similar in cluster and field. Such a rich red spiral population is best explained if quenching is a slow process and morphological transformation is delayed even more. At log M∗/M� < 10, such galaxies are rare, suggesting that their quenching is fast and accompanied by morphological change. We note that edge-on" @default.
- W2097957963 created "2016-06-24" @default.
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- W2097957963 date "2009-03-11" @default.
- W2097957963 modified "2023-10-11" @default.
- W2097957963 title "The STAGES view of red spirals and dusty red galaxies: mass-dependent quenching of star formation in cluster infall" @default.
- W2097957963 cites W1676272010 @default.
- W2097957963 cites W1826794997 @default.
- W2097957963 cites W1965005393 @default.
- W2097957963 cites W1966926090 @default.
- W2097957963 cites W1969920260 @default.
- W2097957963 cites W1970660289 @default.
- W2097957963 cites W1974174849 @default.
- W2097957963 cites W1974772481 @default.
- W2097957963 cites W1974908355 @default.
- W2097957963 cites W1985134004 @default.
- W2097957963 cites W1985370957 @default.
- W2097957963 cites W1985952407 @default.
- W2097957963 cites W1986062018 @default.
- W2097957963 cites W1986537099 @default.
- W2097957963 cites W1987416266 @default.
- W2097957963 cites W1988977670 @default.
- W2097957963 cites W1989910526 @default.
- W2097957963 cites W1993993296 @default.
- W2097957963 cites W1994145175 @default.
- W2097957963 cites W1994244833 @default.
- W2097957963 cites W2000187183 @default.
- W2097957963 cites W2000821703 @default.
- W2097957963 cites W2007325934 @default.
- W2097957963 cites W2009489905 @default.
- W2097957963 cites W2010078196 @default.
- W2097957963 cites W2015295900 @default.
- W2097957963 cites W2016951087 @default.
- W2097957963 cites W2018828554 @default.
- W2097957963 cites W2021008553 @default.
- W2097957963 cites W2028093813 @default.
- W2097957963 cites W2035734390 @default.
- W2097957963 cites W2036056431 @default.
- W2097957963 cites W2045847913 @default.
- W2097957963 cites W2046149262 @default.
- W2097957963 cites W2048758550 @default.
- W2097957963 cites W2055327934 @default.
- W2097957963 cites W205937251 @default.
- W2097957963 cites W2060448616 @default.
- W2097957963 cites W2066773429 @default.
- W2097957963 cites W2068751966 @default.
- W2097957963 cites W2073969519 @default.
- W2097957963 cites W2079227246 @default.
- W2097957963 cites W2087766564 @default.
- W2097957963 cites W2089107762 @default.
- W2097957963 cites W2089167229 @default.
- W2097957963 cites W2094710844 @default.
- W2097957963 cites W2095917766 @default.
- W2097957963 cites W2104899467 @default.
- W2097957963 cites W2108617972 @default.
- W2097957963 cites W2119271505 @default.
- W2097957963 cites W2122666823 @default.
- W2097957963 cites W2124271958 @default.
- W2097957963 cites W2125977823 @default.
- W2097957963 cites W2129662599 @default.
- W2097957963 cites W2129760210 @default.
- W2097957963 cites W2130120613 @default.
- W2097957963 cites W2130164698 @default.
- W2097957963 cites W2134108942 @default.
- W2097957963 cites W2160254914 @default.
- W2097957963 cites W2162290847 @default.
- W2097957963 cites W2167129914 @default.
- W2097957963 cites W2171144488 @default.
- W2097957963 cites W3098135872 @default.
- W2097957963 cites W3098160327 @default.
- W2097957963 cites W3098719395 @default.
- W2097957963 cites W3098813210 @default.
- W2097957963 cites W3099149995 @default.
- W2097957963 cites W3099157579 @default.