paper

Inverse stellar population age gradients of post-starburst galaxies at z=0.8 with LEGA-C

arXiv:2007.00663 · doi:10.1093/mnras/staa1937

Abstract

We use deep, spatially resolved spectroscopy from the LEGA-C 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, and , and find that, on average, PSB galaxies have radially decreasing and increasing profiles. In contrast, a control sample of quiescent, non-PSB galaxies in the same mass range shows outwardly increasing and decreasing . The observed gradients are weak ( Å/), mainly due to seeing convolution. A two-SSP model suggests intrinsic gradients are as strong as observed in local PSB galaxies ( Å). We interpret these results in terms of inside-out growth (for the bulk of the quiescent population) vs star formation occurring last in the centre (for PSB galaxies). At , 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%). 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.

arXiv comment18 pages, 9 figures

References in corpus (134)

Cited by in corpus (26)