How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey
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DOI: 10.1093/mnras/staa2806
Abstract: We investigate how star formation quenching proceeds within central and satellite galaxies using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a complete sample of star formation rate surface densities ($\Sigma_{\rm SFR}$), derived… read more here.
Keywords: satellite galaxies; sigma; central satellite; spectroscopy ... See more keywords