Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
Journal
Monthly Notices of the Royal Astronomical Society
Journal Volume
497
Journal Issue
1
Pages
389-404
Date Issued
2020
Author(s)
D'Eugenio F
van der Wel A
Barone T.M
van Houdt J
Bezanson R
Straatman C.M.S
Pacifici C
Muzzin A
Gallazzi A
Wild V
Sobral D
Bell E.F
Zibetti S
Mowla L
Franx M.
Abstract
We use deep, spatially resolved spectroscopy from the Large Early Galaxy Astrophysics Census Survey to study radial variations in the stellar population of 17 spectroscopically selected post-starburst (PSB) galaxies. We use spectral fitting to measure two Lick indices, H δA and Fe 4383, and find that, on average, PSB galaxies have radially decreasing H δA and increasing Fe 4383 profiles. In contrast, a control sample of quiescent, non-PSB galaxies in the same mass range shows outwardly increasing H δA and decreasing Fe 4383. The observed gradients are weak (≈−0.2 Å/Re), mainly due to seeing convolution. A two-SSP (simple stellar population) model suggests that intrinsic gradients are as strong as observed in local PSB galaxies (≈−0.8 Å/Re). We interpret these results in terms of inside-out growth (for the bulk of the quiescent population) versus star formation occurring last in the centre (for PSB galaxies). At z ≈ 0.8, central starbursts are often the result of gas-rich mergers, as evidenced by the high fraction of PSB galaxies with disturbed morphologies and tidal features (40 per cent). Our results provide additional evidence for multiple paths to quiescence: a standard path, associated with inside-out disc formation and with gradually decreasing star formation activity, without fundamental structural transformation, and a fast path, associated with centrally concentrated starbursts, leaving an inverse age gradient and smaller half-light radius. © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
Subjects
Galaxies: evolution; Galaxies: formation; Galaxies: fundamental parameters; Galaxies: high redshift; Galaxies: starburst; Galaxies: structure
Type
journal article