SDSS-IV MaNGA: the different quenching histories of fast and slow rotators

SDSS-IV MaNGA: the different quenching histories of fast and slow rotators

Do the theorised different formation mechanisms of fast and slow rotators produce an observable difference in their star formation histories? To study this we identify quenching slow rotators in the MaNGA sample by selecting those which lie below the star forming sequence and identify a sample of qu...

Полное описание

Библиографические подробности
Главные авторы:	Smethurst, RJ, Masters, KL, Lintott, CJ, Weijmans, A, Merrifield, M, Penny, SJ, Aragón-Salamanca, A, Brownstein, J, Bundy, K, Drory, N, Law, DR, Nichol, RC
Формат:	Journal article
Опубликовано:	Oxford University Press 2017

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