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SDSS IV MaNGA the spatially resolved transition from star formation to quiescence

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Figure

Figure 1. Example of the different properties of SF (top three), cLIER (middle three) and eLIER (bottom three) galaxies
Figure 2. (a) Density plot in the DN(4000) versus EW(HδA) plane for spaxels in the different galaxy classes (SF, cLIER, eLIER and line-less) defined in thiswork
Figure 3. MaNGA galaxies in the NUV − r versus Mi (colour-magnitude) diagram. Galaxies are divided according the emission-line-based classificationintroduced in Paper I (see also Section 2 of this work)
Table 1. Classification statistics of emission-line galaxies in the NUV − r colour–magnitude diagram and mean (± standard deviation)for selected UV and optical colours
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