The star formation histories of z∼1 post-starburst galaxies

Wild, Vivienne; Aldeen, Laith Taj; Carnall, Adam; Maltby, David; Almaini, Omar; Werle, Ariel; Wilkinson, Aaron; Rowlands, Kate; Bolzonella, Micol; Castellano, Marco; Gargiulo, Adriana; McLure, Ross; Pentericci, Laura; Pozzetti, Lucia

Abstract

We present the star formation histories of 39 galaxies with high-quality rest-frame optical spectra at 0.5 < z < 1.3 selected to have strong Balmer absorption lines and/or Balmer break, and compare to a sample of spectroscopically selected quiescent galaxies at the same redshift. Photometric selection identifies a majority of objects that have clear evidence for a recent short-lived burst of star formation within the last 1.5 Gyr, i.e. ‘post-starburst’ galaxies, however we show that good quality continuum spectra are required to obtain physical parameters such as burst mass fraction and burst age. Dust attenuation appears to be the primary cause for misidentification of post-starburst galaxies, leading to contamination in spectroscopic samples where only the [O ii] emission line is available, as well as a small fraction of objects lost from photometric samples. The 31 confirmed post-starburst galaxies have formed 40–90 per cent of their stellar mass in the last 1–1.5 Gyr. We use the derived star formation histories to find that the post-starburst galaxies are visible photometrically for 0.5–1 Gyr. This allows us to update a previous analysis to suggest that 25–50 per cent of the growth of the red sequence at z ∼ 1 could be caused by a starburst followed by rapid quenching. We use the inferred maximum historical star formation rates of several 100–1000 M⊙ yr−1 and updated visibility times to confirm that sub-mm galaxies are likely progenitors of post-starburst galaxies. The short quenching time-scales of 100–200 Myr are consistent with cosmological hydrodynamic models in which rapid quenching is caused by the mechanical expulsion of gas due to an acive galactic neucleus.

Citation

Wild, V., Aldeen, L. T., Carnall, A., Maltby, D., Almaini, O., Werle, A., …Pozzetti, L. (2020). The star formation histories of z∼1 post-starburst galaxies. Monthly Notices of the Royal Astronomical Society, 494(1), 529–548. https://doi.org/10.1093/mnras/staa674

• Journal Article Type: Article
• Acceptance Date: Mar 5, 2020
• Online Publication Date: Mar 13, 2020
• Publication Date: 2020-05
• Deposit Date: Jan 18, 2021
• Publicly Available Date: Jan 19, 2021
• Journal: Monthly Notices of the Royal Astronomical Society
• Print ISSN: 0035-8711
• Electronic ISSN: 1365-2966
• Publisher: Oxford University Press
• Peer Reviewed: Peer Reviewed
• Volume: 494
• Issue: 1
• Pages: 529–548
• DOI: https://doi.org/10.1093/mnras/staa674
• Keywords: Space and Planetary Science; Astronomy and Astrophysics
• Public URL: https://nottingham-repository.worktribe.com/output/4139519
• Publisher URL: https://academic.oup.com/mnras/article-abstract/494/1/529/5804778?redirectedFrom=fulltext
• Additional Information: This is a pre-copyedited, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The version of record Vivienne Wild, Laith Taj Aldeen, Adam Carnall, David Maltby, Omar Almaini, Ariel Werle, Aaron Wilkinson, Kate Rowlands, Micol Bolzonella, Marco Castellano, Adriana Gargiulo, Ross McLure, Laura Pentericci, Lucia Pozzetti, The star formation histories of z ∼ 1 post-starburst galaxies, Monthly Notices of the Royal Astronomical Society, Volume 494, Issue 1, May 2020, Pages 529–548 is available online at: https://doi.org/10.1093/mnras/staa674