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SDSS IV MaNGA : the spatial distribution of star formation and its dependence on mass, structure and environment

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Figure

Figure 1. The BPT Diagram for galaxies in the MaNGA survey.The positions of galaxies are calculated from the integrated fluxover the entire IFU
Figure 3. We show the star formation rates calculated using justcomposite galaxies in MaNGA
Figure 5. We show the relationships between stellar mass in the left column, group luminosity in the right column, star formation ratein the top row and specific star formation rate in the bottom row, for galaxies with Star forming and Composite BPT types
Figure 6. The radial SSFR profiles in three bins of stellar mass. The individual profiles are shown by the cyan lines and the mean profilein the bin is shown by the solid red line
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