Are galactic star formation and quenching governed by local, global or environmental phenomena?

We present an analysis of star formation and quenching in the SDSS-IV MaNGA-DR15, utilising over 5 million spaxels from ∼3500 local galaxies. We estimate star formation rate surface densities (ΣSFR) via dust corrected Hα flux where possible, and via an empirical relationship between specific star fo...

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society Vol. 492; no. 1; pp. 96 - 139
Main Authors:	Bluck, Asa F. L, Maiolino, Roberto, Sánchez, Sebastian F, Ellison, Sara L, Thorp, Mallory D, Piotrowska, Joanna M, Teimoorinia, Hossen, Bundy, Kevin A
Format:	Journal Article
Language:	English
Published:	United Kingdom Royal Astronomical Society 01.02.2020 OUP Oxford University Press
Subjects:	galaxies: evolution galaxies: formation galaxies: star formation galaxies: statistics galaxies: structure
ISSN:	0035-8711, 1365-2966, 1365-2966
Online Access:	Get full text
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