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Spectroscopic decomposition of the galaxy and halo of the cD galaxy NGC 3311

Johnston, Evelyn J.; Merrifield, Michael; Aragón-Salamanca, Alfonso

Spectroscopic decomposition of the galaxy and halo of the cD galaxy NGC 3311 Thumbnail


Authors

Evelyn J. Johnston

Michael Merrifield



Abstract

Information on the star-formation histories of cD galaxies and their extended stellar haloes lie in their spectra. Therefore, to determine whether these structures evolved together or through a two-phase formation, we need to spectroscopically separate the light from each component. We present a pilot study to use BUDDI to fit and extract the spectra of the cD galaxy NGC 3311 and its halo in an Integral Field Spectroscopy datacube, and carry out a simple stellar populations analysis to study their star-formation histories. Using MUSE data, we were able to isolate the light of the galaxy and its halo throughout the datacube, giving spectra representing purely the light from each of these structures. The stellar populations analysis of the two components indicates that, in this case, the bulk of the stars in both the halo and the central galaxy are very old, but the halo is more metal poor and less α-enriched than the galaxy. This result is consistent with the halo forming through the accretion of much smaller satellite galaxies with more extended star formation. It is noteworthy that the apparent gradients in age and metallicity indicators across the galaxy are entirely consistent with the radially-varying contributions of galaxy and halo components, which individually display no gradients. The success of this study is promising for its application to a larger sample of cD galaxies that are currently being observed by IFU surveys.

Citation

Johnston, E. J., Merrifield, M., & Aragón-Salamanca, A. (in press). Spectroscopic decomposition of the galaxy and halo of the cD galaxy NGC 3311. Monthly Notices of the Royal Astronomical Society, 478(3), https://doi.org/10.1093/mnras/sty1342

Journal Article Type Article
Acceptance Date May 17, 2018
Online Publication Date May 18, 2018
Deposit Date May 30, 2018
Publicly Available Date May 30, 2018
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 478
Issue 3
DOI https://doi.org/10.1093/mnras/sty1342
Keywords galaxies: elliptical and lenticular; cD – galaxies: haloes; galaxies: structure; galaxies: evolution – galaxies: formation; galaxies: individual: NGC 3311
Public URL https://nottingham-repository.worktribe.com/output/932923
Publisher URL https://academic.oup.com/mnras/article/478/3/4255/4999936
Additional Information This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

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