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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Published in | Monthly notices of the Royal Astronomical Society Vol. 499; no. 1; pp. 230 - 268 |
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Main Authors | , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
United Kingdom
Oxford University Press
01.11.2020
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Subjects | |
Online Access | Get full text |
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