Post-starburst properties of post-merger galaxies
Abstract
ABSTRACT Post-starburst galaxies (PSBs) are transition galaxies showing evidence of recent rapid star formation quenching. To understand the role of galaxy mergers in triggering quenching, we investigate the incidence of PSBs and resolved PSB properties in post-merger galaxies using both SDSS single-fibre spectra and MaNGA resolved IFU spectra. We find post-mergers have a PSB excess of 10–20 times that relative to their control galaxies using single-fibre PSB diagnostics. A similar excess of ∼ 19 times is also found in the fraction of central (C)PSBs and ring-like (R)PSBs in post-mergers using the resolved PSB diagnostic. However, 60 per cent of the CPSBs + RPSBs in both post-mergers and control galaxies are missed by the single-fibre data. By visually inspecting the resolved PSB distribution, we find that the fraction of outside-in quenching is seven times higher than inside-out quenching in PSBs in post-mergers while PSBs in control galaxies do not show large differences in these quenching directions. In addition, we find a marginal deficit of H i gas in PSBs relative to non-PSBs in post-mergers using the MaNGA-H i data. The excesses of PSBs in post-mergers suggest that mergers play an important role in triggering quenching. Resolved IFU spectra are important to recover the PSBs missed by single-fibre spectra. The excessmore »
- Publication Date:
- Sponsoring Org.:
- USDOE
- OSTI Identifier:
- 1975298
- Resource Type:
- Published Article
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Name: Monthly Notices of the Royal Astronomical Society Journal Volume: 523 Journal Issue: 1; Journal ID: ISSN 0035-8711
- Publisher:
- Oxford University Press
- Country of Publication:
- United Kingdom
- Language:
- English
Citation Formats
Li, Wenhao, Nair, Preethi, Rowlands, Kate, Masters, Karen, Stark, David, Drory, Niv, Ellison, Sara, Irwin, Jimmy, Satyapal, Shobita, Jones, Amy, Keel, William, Mukundan, Kavya, and Tu, Zachary. Post-starburst properties of post-merger galaxies. United Kingdom: N. p., 2023.
Web. doi:10.1093/mnras/stad1473.
Li, Wenhao, Nair, Preethi, Rowlands, Kate, Masters, Karen, Stark, David, Drory, Niv, Ellison, Sara, Irwin, Jimmy, Satyapal, Shobita, Jones, Amy, Keel, William, Mukundan, Kavya, & Tu, Zachary. Post-starburst properties of post-merger galaxies. United Kingdom. https://doi.org/10.1093/mnras/stad1473
Li, Wenhao, Nair, Preethi, Rowlands, Kate, Masters, Karen, Stark, David, Drory, Niv, Ellison, Sara, Irwin, Jimmy, Satyapal, Shobita, Jones, Amy, Keel, William, Mukundan, Kavya, and Tu, Zachary. Tue .
"Post-starburst properties of post-merger galaxies". United Kingdom. https://doi.org/10.1093/mnras/stad1473.
@article{osti_1975298,
title = {Post-starburst properties of post-merger galaxies},
author = {Li, Wenhao and Nair, Preethi and Rowlands, Kate and Masters, Karen and Stark, David and Drory, Niv and Ellison, Sara and Irwin, Jimmy and Satyapal, Shobita and Jones, Amy and Keel, William and Mukundan, Kavya and Tu, Zachary},
abstractNote = {ABSTRACT Post-starburst galaxies (PSBs) are transition galaxies showing evidence of recent rapid star formation quenching. To understand the role of galaxy mergers in triggering quenching, we investigate the incidence of PSBs and resolved PSB properties in post-merger galaxies using both SDSS single-fibre spectra and MaNGA resolved IFU spectra. We find post-mergers have a PSB excess of 10–20 times that relative to their control galaxies using single-fibre PSB diagnostics. A similar excess of ∼ 19 times is also found in the fraction of central (C)PSBs and ring-like (R)PSBs in post-mergers using the resolved PSB diagnostic. However, 60 per cent of the CPSBs + RPSBs in both post-mergers and control galaxies are missed by the single-fibre data. By visually inspecting the resolved PSB distribution, we find that the fraction of outside-in quenching is seven times higher than inside-out quenching in PSBs in post-mergers while PSBs in control galaxies do not show large differences in these quenching directions. In addition, we find a marginal deficit of H i gas in PSBs relative to non-PSBs in post-mergers using the MaNGA-H i data. The excesses of PSBs in post-mergers suggest that mergers play an important role in triggering quenching. Resolved IFU spectra are important to recover the PSBs missed by single-fibre spectra. The excess of outside-in quenching relative to inside-out quenching in post-mergers suggests that AGNs are not the dominant quenching mechanism in these galaxies, but that processes from the disc (gas inflows/consumption and stellar feedback) play a more important role.},
doi = {10.1093/mnras/stad1473},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 1,
volume = 523,
place = {United Kingdom},
year = {Tue May 16 00:00:00 EDT 2023},
month = {Tue May 16 00:00:00 EDT 2023}
}
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