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...

Celý popis

Podrobná bibliografia

Vydané v:	Monthly notices of the Royal Astronomical Society Ročník 492; číslo 1; s. 96 - 139
Hlavní autori:	Bluck, Asa F. L, Maiolino, Roberto, Sánchez, Sebastian F, Ellison, Sara L, Thorp, Mallory D, Piotrowska, Joanna M, Teimoorinia, Hossen, Bundy, Kevin A
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	United Kingdom Royal Astronomical Society 01.02.2020 OUP Oxford University Press
Predmet:	galaxies: evolution galaxies: formation galaxies: star formation galaxies: statistics galaxies: structure
ISSN:	0035-8711, 1365-2966, 1365-2966
On-line prístup:	Získať plný text
Tagy:	Pridať tag Žiadne tagy, Buďte prvý, kto otaguje tento záznam!