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On the accretion of a new group of galaxies on to Virgo – II. The effect of pre-processing on the stellar population content of dEs

Bidaran, Bahar; La Barbera, Francesco; Pasquali, Anna; Peletier, Reynier; van de Ven, Glenn; Grebel, Eva K; Falcón-Barroso, Jesus; Sybilska, Agnieszka; Gadotti, Dimitri A; Coccato, Lodovico

On the accretion of a new group of galaxies on to Virgo – II. The effect of pre-processing on the stellar population content of dEs Thumbnail


Authors

Bahar Bidaran

Francesco La Barbera

Anna Pasquali

Reynier Peletier

Glenn van de Ven

Eva K Grebel

Jesus Falcón-Barroso

Agnieszka Sybilska

Lodovico Coccato



Abstract

Using MUSE spectra, we investigate how pre-processing and accretion on to a galaxy cluster affect the integrated stellar population properties of dwarf early-type galaxies (dEs). We analyse a sample of nine dEs with stellar masses of ∼109M⊙⁠, which were accreted (∼ 2–3 Gyr ago) on to the Virgo cluster as members of a massive galaxy group. We derive their stellar population properties, namely age, metallicity ([M/H]), and the abundance ratio of α elements ([α/Fe]), by fitting observed spectral indices with a robust, iterative procedure, and infer their star formation history (SFH) by means of full spectral fitting. We find that these nine dEs are more metal-poor (at the 2–3σ level) and significantly more α-enhanced than dEs in the Virgo and Coma clusters with similar stellar mass, clustercentric distance, and infall time. Moreover, for six dEs, we find evidence for a recent episode of star formation during or right after the time of accretion on to Virgo. We interpret the high [α/Fe] of our sample of dEs as the result of the previous exposure of these galaxies to an environment hostile to star formation, and/or the putative short burst of star formation they underwent after infall into Virgo. Our results suggest that the stellar population properties of low-mass galaxies may be the result of the combined effect of pre-processing in galaxy groups and environmental processes (such as ram-pressure triggering star formation) acting during the early phases of accretion on to a cluster.

Citation

Bidaran, B., La Barbera, F., Pasquali, A., Peletier, R., van de Ven, G., Grebel, E. K., Falcón-Barroso, J., Sybilska, A., Gadotti, D. A., & Coccato, L. (2022). On the accretion of a new group of galaxies on to Virgo – II. The effect of pre-processing on the stellar population content of dEs. Monthly Notices of the Royal Astronomical Society, 515(3), 4622-4638. https://doi.org/10.1093/mnras/stac2005

Journal Article Type Article
Acceptance Date Jul 13, 2022
Online Publication Date Jul 22, 2022
Publication Date 2022-09
Deposit Date Sep 15, 2022
Publicly Available Date Sep 22, 2022
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 515
Issue 3
Pages 4622-4638
DOI https://doi.org/10.1093/mnras/stac2005
Public URL https://durham-repository.worktribe.com/output/1191721

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Copyright Statement
This article has been accepted for publication in Monthly notices of the Royal Astronomical Society. ©: 2022 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.






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