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 in:	Monthly 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
Language:	English
Published:	United Kingdom Oxford University Press 01.11.2020
Subjects:	galaxies: formation Galaxy: bulge Galaxy: disc galaxies: evolution galaxies: statistics galaxies: star formation
ISSN:	0035-8711, 1365-2966
Online Access:	Get full text
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