SDSS-IV MaNGA: The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies

Kexin Guo, Yingjie Peng, Li Shao, Hai Fu, Barbara Catinella, Luca Cortese, Feng Yuan, Renbin Yan, Chengpeng Zhang, Jing Dou

Research output: Contribution to journalArticle

2 Citations (Scopus)

Abstract

We study how star formation (SF) is quenched in low-redshift disk galaxies with integral-field spectroscopy. We select 131 face-on spiral galaxies with stellar mass greater than 3 x 10(10) M-circle dot, and with spatially resolved spectrum from MaNGA DR13. We subdivide the sample into four groups based on the offset of their global specific star formation rate (SFR) from the star-forming main sequence and stack the radial profiles of stellar mass and SFR. By comparing the stacked profiles of quiescent and star-forming disk galaxies, we find that the decrease of the global SFR is caused by the suppression of SF at all radii, but with a more significant drop from the center to the outer regions following an inside-out pattern. As the global specific SFR decreases, the central stellar mass, the fraction of disk galaxies hosting stellar bars, and active galactic nuclei (AGNs; including both LINERs and Seyferts) all increase, indicating dynamical processes and AGN feedback are possible contributors to the inside-out quenching of SF in the local universe. However, if we include only Seyferts, or AGNs with EW(H alpha) > 3 angstrom, the increasing trend of AGN fraction with decreasing global sSFR disappears. Therefore, if AGN feedback is contributing to quenching, we suspect that it operates in the low-luminosity AGN mode, as indicated by the increasing large bulge mass of the more passive disk galaxies.

Original languageEnglish
Article number19
Number of pages11
JournalAstrophysical Journal
Volume870
Issue number1
DOIs
Publication statusPublished - 1 Jan 2019

Cite this

Guo, Kexin ; Peng, Yingjie ; Shao, Li ; Fu, Hai ; Catinella, Barbara ; Cortese, Luca ; Yuan, Feng ; Yan, Renbin ; Zhang, Chengpeng ; Dou, Jing. / SDSS-IV MaNGA : The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies. In: Astrophysical Journal. 2019 ; Vol. 870, No. 1.
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abstract = "We study how star formation (SF) is quenched in low-redshift disk galaxies with integral-field spectroscopy. We select 131 face-on spiral galaxies with stellar mass greater than 3 x 10(10) M-circle dot, and with spatially resolved spectrum from MaNGA DR13. We subdivide the sample into four groups based on the offset of their global specific star formation rate (SFR) from the star-forming main sequence and stack the radial profiles of stellar mass and SFR. By comparing the stacked profiles of quiescent and star-forming disk galaxies, we find that the decrease of the global SFR is caused by the suppression of SF at all radii, but with a more significant drop from the center to the outer regions following an inside-out pattern. As the global specific SFR decreases, the central stellar mass, the fraction of disk galaxies hosting stellar bars, and active galactic nuclei (AGNs; including both LINERs and Seyferts) all increase, indicating dynamical processes and AGN feedback are possible contributors to the inside-out quenching of SF in the local universe. However, if we include only Seyferts, or AGNs with EW(H alpha) > 3 angstrom, the increasing trend of AGN fraction with decreasing global sSFR disappears. Therefore, if AGN feedback is contributing to quenching, we suspect that it operates in the low-luminosity AGN mode, as indicated by the increasing large bulge mass of the more passive disk galaxies.",
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SDSS-IV MaNGA : The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies. / Guo, Kexin; Peng, Yingjie; Shao, Li; Fu, Hai; Catinella, Barbara; Cortese, Luca; Yuan, Feng; Yan, Renbin; Zhang, Chengpeng; Dou, Jing.

In: Astrophysical Journal, Vol. 870, No. 1, 19, 01.01.2019.

Research output: Contribution to journalArticle

TY - JOUR

T1 - SDSS-IV MaNGA

T2 - The Roles of AGNs and Dynamical Processes in Star Formation Quenching in Nearby Disk Galaxies

AU - Guo, Kexin

AU - Peng, Yingjie

AU - Shao, Li

AU - Fu, Hai

AU - Catinella, Barbara

AU - Cortese, Luca

AU - Yuan, Feng

AU - Yan, Renbin

AU - Zhang, Chengpeng

AU - Dou, Jing

PY - 2019/1/1

Y1 - 2019/1/1

N2 - We study how star formation (SF) is quenched in low-redshift disk galaxies with integral-field spectroscopy. We select 131 face-on spiral galaxies with stellar mass greater than 3 x 10(10) M-circle dot, and with spatially resolved spectrum from MaNGA DR13. We subdivide the sample into four groups based on the offset of their global specific star formation rate (SFR) from the star-forming main sequence and stack the radial profiles of stellar mass and SFR. By comparing the stacked profiles of quiescent and star-forming disk galaxies, we find that the decrease of the global SFR is caused by the suppression of SF at all radii, but with a more significant drop from the center to the outer regions following an inside-out pattern. As the global specific SFR decreases, the central stellar mass, the fraction of disk galaxies hosting stellar bars, and active galactic nuclei (AGNs; including both LINERs and Seyferts) all increase, indicating dynamical processes and AGN feedback are possible contributors to the inside-out quenching of SF in the local universe. However, if we include only Seyferts, or AGNs with EW(H alpha) > 3 angstrom, the increasing trend of AGN fraction with decreasing global sSFR disappears. Therefore, if AGN feedback is contributing to quenching, we suspect that it operates in the low-luminosity AGN mode, as indicated by the increasing large bulge mass of the more passive disk galaxies.

AB - We study how star formation (SF) is quenched in low-redshift disk galaxies with integral-field spectroscopy. We select 131 face-on spiral galaxies with stellar mass greater than 3 x 10(10) M-circle dot, and with spatially resolved spectrum from MaNGA DR13. We subdivide the sample into four groups based on the offset of their global specific star formation rate (SFR) from the star-forming main sequence and stack the radial profiles of stellar mass and SFR. By comparing the stacked profiles of quiescent and star-forming disk galaxies, we find that the decrease of the global SFR is caused by the suppression of SF at all radii, but with a more significant drop from the center to the outer regions following an inside-out pattern. As the global specific SFR decreases, the central stellar mass, the fraction of disk galaxies hosting stellar bars, and active galactic nuclei (AGNs; including both LINERs and Seyferts) all increase, indicating dynamical processes and AGN feedback are possible contributors to the inside-out quenching of SF in the local universe. However, if we include only Seyferts, or AGNs with EW(H alpha) > 3 angstrom, the increasing trend of AGN fraction with decreasing global sSFR disappears. Therefore, if AGN feedback is contributing to quenching, we suspect that it operates in the low-luminosity AGN mode, as indicated by the increasing large bulge mass of the more passive disk galaxies.

KW - galaxies: active

KW - galaxies: evolution

KW - galaxies: star formation

KW - galaxies: structure

KW - SIMILAR-TO 3

KW - MORPHOLOGICAL CLASSIFICATIONS

KW - SECULAR EVOLUTION

KW - FORMATION HISTORIES

KW - FORMING GALAXIES

KW - SPIRAL GALAXIES

KW - BARRED GALAXIES

KW - STELLAR MASSES

KW - HOST GALAXIES

KW - LINE SPECTRA

U2 - 10.3847/1538-4357/aaee88

DO - 10.3847/1538-4357/aaee88

M3 - Article

VL - 870

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 19

ER -