Bahar Bidaran
On the accretion of a new group of galaxies onto Virgo – III. The stellar population radial gradients of dEs
Bidaran, Bahar; La Barbera, Francesco; Pasquali, Anna; van de Ven, Glenn; Peletier, Reynier; Falcón-Barroso, Jesus; Gadotti, Dimitri A; Sybilska, Agnieszka; Grebel, Eva K
Authors
Francesco La Barbera
Anna Pasquali
Glenn van de Ven
Reynier Peletier
Jesus Falcón-Barroso
Dr Dimitri Gadotti dimitri.a.gadotti@durham.ac.uk
Assistant Professor
Agnieszka Sybilska
Eva K Grebel
Abstract
Using MUSE data, we investigate the radial gradients of stellar population properties (namely age, [M/H], and the abundance ratio of α elements [α/Fe]) for a sample of nine dwarf early-type (dE) galaxies with log(M/M) ∼ 9.0 and an infall time onto the Virgo cluster of 2–3 Gyr ago. We followed a similar approach as in Bidaran et al. to derive their stellar population properties and star formation histories (SFHs) through fitting observed spectral indices and full spectral fitting, respectively. We find that these nine dE galaxies have truncated [Mg/Fe] versus [Fe/H] profiles than equally massive Virgo dE galaxies with longer past infall times. Short profiles of three dE galaxies are the result of their intense star formation which has been quenched long before their accretion onto the Virgo cluster, possibly as a result of their group environment. In the remaining six dE galaxies, profiles
mainly trace a recent episode of star burst within 0.4Re which results in higher light-weighted [α/Fe] values. The latter SFH peak can be due to ram pressure exerted by the Virgo cluster at the time of the accretion of the dE galaxies. Also, we show that younger, more metal-rich, and less α-enhanced stellar populations dominate their inner regions (i.e. < 0.4Re) resulting in mainly flat ∇age, negative ∇[M/H], and positive ∇[α/Fe]. We find that with increasing log(σ Re) of dE galaxies, ∇age and ∇[α/Fe] flatten, and the latter correlation persists even after including early-type galaxies up to log(σ Re ∼ 2.5), possibly due to the more extended star formation activity in the inner regions of dEs, as opposed to more massive early-type galaxies.
Citation
Bidaran, B., La Barbera, F., Pasquali, A., van de Ven, G., Peletier, R., Falcón-Barroso, J., …Grebel, E. K. (2023). On the accretion of a new group of galaxies onto Virgo – III. The stellar population radial gradients of dEs. Monthly Notices of the Royal Astronomical Society, 525(3), 4329–4346. https://doi.org/10.1093/mnras/stad2546
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 16, 2023 |
Online Publication Date | Aug 31, 2023 |
Publication Date | 2023-11 |
Deposit Date | Jan 30, 2024 |
Publicly Available Date | Jan 30, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 525 |
Issue | 3 |
Pages | 4329–4346 |
DOI | https://doi.org/10.1093/mnras/stad2546 |
Public URL | https://durham-repository.worktribe.com/output/2187182 |
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