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Fornax3D project: Assembly history of massive early-type galaxies in the Fornax cluster from deep imaging and integral field spectroscopy

Spavone, M.; Iodice, E.; D’Ago, G.; van de Ven, G.; Morelli, L.; Corsini, E.M.; Sarzi, M.; Coccato, L.; Fahrion, K.; Falcón-Barroso, J.; Gadotti, D.A.; Lyubenova, M.; Martín-Navarro, I.; McDermid, R.M.; Pinna, F.; Pizzella, A.; Poci, A.; de Zeeuw, P.T.; Zhu, L.

Fornax3D project: Assembly history of massive early-type galaxies in the Fornax cluster from deep imaging and integral field spectroscopy Thumbnail


Authors

M. Spavone

E. Iodice

G. D’Ago

G. van de Ven

L. Morelli

E.M. Corsini

M. Sarzi

L. Coccato

K. Fahrion

J. Falcón-Barroso

D.A. Gadotti

M. Lyubenova

I. Martín-Navarro

R.M. McDermid

F. Pinna

A. Pizzella

P.T. de Zeeuw

L. Zhu



Abstract

This work is based on high-quality integral-field spectroscopic data obtained with the Multi Unit Spectroscopic Explorer (MUSE) on the Very Large Telescope (VLT). The 21 brightest (mB ≤ 15 mag) early-type galaxies (ETGs) inside the virial radius of the Fornax cluster are observed out to distances of ∼2−3 Re. Deep imaging from the VLT Survey Telescope (VST) is also available for the sample ETGs. We investigated the variation of the galaxy structural properties as a function of the total stellar mass and cluster environment. Moreover, we correlated the size scales of the luminous components derived from a multi-component decomposition of the VST surface-brightness radial profiles of the sample ETGs with the MUSE radial profiles of stellar kinematic and population properties. The results are compared with both theoretical predictions and previous observational studies and used to address the assembly history of the massive ETGs of the Fornax cluster. We find that galaxies in the core and north-south clump of the cluster, which have the highest accreted mass fraction, show milder metallicity gradients in their outskirts than the galaxies infalling into the cluster. We also find a segregation in both age and metallicity between the galaxies belonging to the core and north-south clump and the infalling galaxies. The new findings fit well within the general framework for the assembly history of the Fornax cluster.

Citation

Spavone, M., Iodice, E., D’Ago, G., van de Ven, G., Morelli, L., Corsini, E., Sarzi, M., Coccato, L., Fahrion, K., Falcón-Barroso, J., Gadotti, D., Lyubenova, M., Martín-Navarro, I., McDermid, R., Pinna, F., Pizzella, A., Poci, A., de Zeeuw, P., & Zhu, L. (2022). Fornax3D project: Assembly history of massive early-type galaxies in the Fornax cluster from deep imaging and integral field spectroscopy. Astronomy & Astrophysics, 663, Article A135. https://doi.org/10.1051/0004-6361/202243290

Journal Article Type Article
Acceptance Date May 27, 2022
Online Publication Date Jul 20, 2022
Publication Date 2022-07
Deposit Date Aug 19, 2022
Publicly Available Date Aug 19, 2022
Journal Astronomy and astrophysics.
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 663
Article Number A135
DOI https://doi.org/10.1051/0004-6361/202243290
Public URL https://durham-repository.worktribe.com/output/1196554

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0),
which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.






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