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- W2896579862 abstract "We present a study of the integrated properties of the 835 galaxies in the CALIFA survey. To derive the main physical parameters of the galaxies we have fitted their UV-to-IR spectral energy distributions (SED) with sets of theoretical models using CIGALE. We perform a comparison of the integrated galaxy parameters derived from multi-band SED fitting with those obtained from modelling the Integral Field Unit (IFU) spectra and show the clear advantage of using the SED-derived star formation rates (SFR). A detailed analysis of galaxies in the SFR/Mstar plane as a function of their properties reveals that quenching of star formation is caused by a combination of gas deficiency and the inefficiency of the existing gas to form new stars. Exploring the plausible mechanisms that could produce this effect, we find a strong correlation with galaxy morphology and the build-up of central bulge. On the other hand, the presence of AGN and/or a stellar bar, as well as the local environment have only temporal effects on the current star formation, a result also consistent with their model-derived star formation histories." @default.
- W2896579862 created "2018-10-26" @default.
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- W2896579862 date "2018-10-23" @default.
- W2896579862 modified "2023-10-18" @default.
- W2896579862 title "The integrated properties of the CALIFA galaxies: model-derived galaxy parameters and quenching of star formation" @default.
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- W2896579862 doi "https://doi.org/10.1093/mnras/sty2857" @default.
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