4.7 Article

The merger fraction of post-starburst galaxies in UNIONS

期刊

出版社

OXFORD UNIV PRESS
DOI: 10.1093/mnras/stac1962

关键词

galaxies: evolution; galaxies: interactions; galaxies: starburst; galaxies: structure

资金

  1. Natural Sciences and Engineering Council of Canada (NSERC) [PDF-546234-2020]
  2. STFC [ST/V000861/1]
  3. Canadian Space Agency
  4. NASA SSO Near Earth Observation Program [80NSSC18K0971, NNX14AM74G, NNX12AR65G, NNX13AQ47G, NNX08AR22G, YORPD20 2-0014]
  5. State of Hawaii
  6. Alfred P. Sloan Foundation
  7. National Science Foundation
  8. U.S. Department of Energy
  9. National Aeronautics and Space Administration
  10. Japanese Monbukagakusho
  11. Max Planck Society
  12. Higher Education Funding Council for England
  13. American Museum of Natural History
  14. Astrophysical Institute Potsdam
  15. University of Basel
  16. University of Cambridge
  17. Case Western Reserve University
  18. University of Chicago
  19. Drexel University
  20. Fermilab
  21. Institute for Advanced Study
  22. Japan Participation Group
  23. Johns Hopkins University
  24. Joint Institute for Nuclear Astrophysics
  25. Kavli Institute for Particle Astrophysics and Cosmology
  26. Korean Scientist Group
  27. Chinese Academy of Sciences (LAMOST)
  28. Los Alamos National Laboratory
  29. Max-Planck-Institute for Astronomy (MPIA)
  30. MaxPlanck-Institute for Astrophysics (MPA)
  31. New Mexico State University
  32. Ohio State University
  33. University of Pittsburgh
  34. University of Portsmouth
  35. Princeton University
  36. United States Naval Observatory
  37. University of Washington

向作者/读者索取更多资源

Merger plays a significant role in generating post-starburst galaxies (PSBs), but other mechanisms are also required. However, the detection rate of post-merger galaxies is relatively low, suggesting that nearly all PSBs might have undergone a merger in their recent past.
Post-starburst galaxies (PSBs) are defined as having experienced a recent burst of star formation, followed by a prompt truncation in further activity. Identifying the mechanism(s) causing a galaxy to experience a post-starburst phase therefore provides integral insight into the causes of rapid quenching. Galaxy mergers have long been proposed as a possible post-starburst trigger. Effectively testing this hypothesis requires a large spectroscopic galaxy survey to identify the rare PSBs as well as high-quality imaging and robust morphology metrics to identify mergers. We bring together these critical elements by selecting PSBs from the overlap of the Sloan Digital Sky Survey and the Canada-France Imaging Survey and applying a suite of classification methods: non-parametric morphology metrics such as asymmetry and Gini-M-20, a convolutional neural network trained to identify post-merger galaxies, and visual classification. This work is therefore the largest and most comprehensive assessment of the merger fraction of PSBs to date. We find that the merger fraction of PSBs ranges from 19 per cent to 42 per cent depending on the merger identification method and details of the PSB sample selection. These merger fractions represent an excess of 3-46x relative to non-PSB control samples. Our results demonstrate that mergers play a significant role in generating PSBs, but that other mechanisms are also required. However, applying our merger identification metrics to known post-mergers in the IllustrisTNG simulation shows that 70 per cent of recent post-mergers (less than or similar to 200 Myr) would not be detected. Thus, we cannot exclude the possibility that nearly all PSBs have undergone a merger in their recent past.

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