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

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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...

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Bibliographic Details
Main Authors:	Smethurst, Rebecca J., Masters, Karen L., Lintott, Chris J., Weijmans, Anne-Marie, Merrifield, Michael R., Penny, Samantha J., Aragón-Salamanca, Alfonso, Brownstein, J., Bundy, Kevin, Drory, Niv, Law, D.R., Nichol, Robert C.
Format:	Article
Published:	Oxford University Press 2018
Subjects:	galaxies-photometry galaxies-statistics galaxies-morphology
Online Access:	https://eprints.nottingham.ac.uk/47084/

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