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Rejuvenation triggers nuclear activity in nearby galaxies

Rejuvenation triggers nuclear activity in nearby galaxies
Rejuvenation triggers nuclear activity in nearby galaxies
Feedback, in particular from active galactic nuclei (AGNs), is believed to play a crucial role in the evolution of galaxies. In the local Universe, many galaxies with an AGN are indeed observed to reside in the so-called green valley, usually interpreted as a transition phase from a blue star-forming to a red quenched state. We use data from the Sloan Digital Sky Survey to show that such an interpretation requires substantial revision. Optically selected nearby AGN galaxies follow exponentially declining star formation histories, as normal galaxies of similar stellar and dark matter halo mass, reaching in the recent past (∼0.1 Gyr ago) star formation rate levels consistent with a quiescent population. However, we find that local AGN galaxies have experienced a sudden increase in their star formation rate, unfolding on time-scales similar to those typical of AGN activity, suggesting that both star formation and AGN activity were triggered simultaneously. We find that this quenching followed by an enhancement in the star formation rate is common to AGN galaxies and more pronounced in early-type galaxies. Our results demonstrate that local AGN galaxies are not just a simple transition type between star-forming and quiescent galaxies as previously postulated.
1745-3925
L10–L14
Martin-Navarro, Ignacio
39dd8f48-4a9e-400c-b37d-2d26d106e810
Shankar, F.
b10c91e4-85cd-4394-a18a-d4f049fd9cdb
Mezcua, Mar
39cb729d-b438-4d63-95f2-3c318ff87ad1
Martin-Navarro, Ignacio
39dd8f48-4a9e-400c-b37d-2d26d106e810
Shankar, F.
b10c91e4-85cd-4394-a18a-d4f049fd9cdb
Mezcua, Mar
39cb729d-b438-4d63-95f2-3c318ff87ad1

Martin-Navarro, Ignacio, Shankar, F. and Mezcua, Mar (2021) Rejuvenation triggers nuclear activity in nearby galaxies. Monthly Notices of the Royal Astronomical Society: Letters, 513 (1), L10–L14. (doi:10.1093/mnrasl/slab112).

Record type: Article

Abstract

Feedback, in particular from active galactic nuclei (AGNs), is believed to play a crucial role in the evolution of galaxies. In the local Universe, many galaxies with an AGN are indeed observed to reside in the so-called green valley, usually interpreted as a transition phase from a blue star-forming to a red quenched state. We use data from the Sloan Digital Sky Survey to show that such an interpretation requires substantial revision. Optically selected nearby AGN galaxies follow exponentially declining star formation histories, as normal galaxies of similar stellar and dark matter halo mass, reaching in the recent past (∼0.1 Gyr ago) star formation rate levels consistent with a quiescent population. However, we find that local AGN galaxies have experienced a sudden increase in their star formation rate, unfolding on time-scales similar to those typical of AGN activity, suggesting that both star formation and AGN activity were triggered simultaneously. We find that this quenching followed by an enhancement in the star formation rate is common to AGN galaxies and more pronounced in early-type galaxies. Our results demonstrate that local AGN galaxies are not just a simple transition type between star-forming and quiescent galaxies as previously postulated.

Text
2110.04305 - Accepted Manuscript
Available under License Creative Commons Attribution.
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e-pub ahead of print date: 30 March 2021
Additional Information: arXiv:2110.04305

Identifiers

Local EPrints ID: 457498
URI: http://eprints.soton.ac.uk/id/eprint/457498
ISSN: 1745-3925
PURE UUID: 07b88d69-5a6c-441a-9edc-ca20a480c031

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Date deposited: 09 Jun 2022 17:08
Last modified: 16 Mar 2024 17:33

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Contributors

Author: Ignacio Martin-Navarro
Author: F. Shankar
Author: Mar Mezcua

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