SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment

SDSS-IV MaNGA: stellar population gradients as a function of galaxy environment

We study the internal radial gradients of stellar population properties within 1.5 Re and analyse the impact of galaxy environment. We use a representative sample of 721 galaxies with masses ranging between 109 M⊙ and 1011.5 M⊙ from the SDSS-IV survey MaNGA. We split this sample by morphology into e...

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Bibliographic Details
Main Authors: Goddard, D., Thomas, D., Maraston, C., Westfall, K., Etherington, J., Riffel, R., Mallmann, N.D., Zheng, Z., Argudo-Fernández, M., Bershady, M., Bundy, K., Drory, N., Law, D., Yan, R., Wake, D., Weijmans, A., Bizyaev, D., Brownstein, J., Lane, R.R., Maiolino, R., Masters, K., Merrifield, M., Nitschelm, C., Pan, K., Roman-Lopes, A., Storchi-Bergmann, T.
Format: Article
Published: Oxford University Press 2017
Subjects:
surveys
galaxies: elliptical and lenticular
cD
galaxies: evolution
galaxies: formation
galaxies: spiral
galaxies: stellar content
Online Access:https://eprints.nottingham.ac.uk/41596/

Internet

https://eprints.nottingham.ac.uk/41596/

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