How do central and satellite galaxies quench? – Insights from spatially resolved spectroscopy in the MaNGA survey

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 (ΣSFR), derived in Bluck et al. (2020), to compute the distance a...

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Bibliographic Details
Published inMonthly notices of the Royal Astronomical Society Vol. 499; no. 1; pp. 230 - 268
Main Authors Bluck, Asa F L, Maiolino, Roberto, Piotrowska, Joanna M, Trussler, James, Ellison, Sara L, Sánchez, Sebastian F, Thorp, Mallory D, Teimoorinia, Hossen, Moreno, Jorge, Conselice, Christopher J
Format Journal Article
LanguageEnglish
Published United Kingdom Oxford University Press 01.11.2020
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