The local universe in the era of large surveys – III. radial activity profiles of S0 galaxies
The local universe in the era of large surveys – III. radial activity profiles of S0 galaxies
Spatially resolved MaNGA’s optical spectra of 1072 present-day lenticular (S0) galaxies, dimensionally reduced from a principal component analysis (PCA), are used to determine their radial activity structure shaped by any possible nebular ionization source. Activity profiles within 1.5 R e are examined in tandem with the mass, age, ellipticity, and kinematics of the stars, as well as environmental density. Among the results of this comparison, we find that the sign of the radial activity gradient of S0s is tightly related to their PCA classification, BPT designation, and star formation status. PCA-passive lenticulars often show low-level, flat activity profiles, although there is also a significant number of systems with positive gradients, while their less common active counterparts generally have negative gradients, usually associated with high SSFRs and, sometimes, moderate Seyfert emission. A fraction of the latter also shows radial activity profiles with positive gradients, which become more abundant with increasing stellar mass regardless of environmental density. Our analysis also reveals that the subset of active S0s with negative gradients experiences at all galactocentric radii a systematic reduction in its median activity level with stellar mass, consistent with expectations for main-sequence galaxies. In contrast, passive S0s with positive gradients show the opposite behaviour. Furthermore, systems whose activity is dominated by star formation are structurally rounder than the rest of S0s, while those classified as Seyfert exhibit higher rotational support. The possibility that negative and positive activity gradients in S0s may result from rejuvenation by two distinct types of minor mergers is raised.
galaxies: Seyfert, galaxies: active, galaxies: elliptical and lenticular, cD, galaxies: evolution, galaxies: star formation, galaxies: statistics
3260-3280
Tous, J.L.
53e68ff4-8401-4d43-9ed2-f8b4c7b1fd53
Solanes, J.M.
b235e56b-b858-4305-969d-2c7cface62f5
Perea, J.D.
2404daec-51cd-4f06-9e84-29c2301af062
Domínguez-Sánchez, H.
718e2374-5004-4a73-b95e-77e819f3abea
2 February 2024
Tous, J.L.
53e68ff4-8401-4d43-9ed2-f8b4c7b1fd53
Solanes, J.M.
b235e56b-b858-4305-969d-2c7cface62f5
Perea, J.D.
2404daec-51cd-4f06-9e84-29c2301af062
Domínguez-Sánchez, H.
718e2374-5004-4a73-b95e-77e819f3abea
Tous, J.L., Solanes, J.M., Perea, J.D. and Domínguez-Sánchez, H.
(2024)
The local universe in the era of large surveys – III. radial activity profiles of S0 galaxies.
Monthly Notices Of The Royal Astronomical Society, 528 (2), .
(doi:10.1093/mnras/stae097).
Abstract
Spatially resolved MaNGA’s optical spectra of 1072 present-day lenticular (S0) galaxies, dimensionally reduced from a principal component analysis (PCA), are used to determine their radial activity structure shaped by any possible nebular ionization source. Activity profiles within 1.5 R e are examined in tandem with the mass, age, ellipticity, and kinematics of the stars, as well as environmental density. Among the results of this comparison, we find that the sign of the radial activity gradient of S0s is tightly related to their PCA classification, BPT designation, and star formation status. PCA-passive lenticulars often show low-level, flat activity profiles, although there is also a significant number of systems with positive gradients, while their less common active counterparts generally have negative gradients, usually associated with high SSFRs and, sometimes, moderate Seyfert emission. A fraction of the latter also shows radial activity profiles with positive gradients, which become more abundant with increasing stellar mass regardless of environmental density. Our analysis also reveals that the subset of active S0s with negative gradients experiences at all galactocentric radii a systematic reduction in its median activity level with stellar mass, consistent with expectations for main-sequence galaxies. In contrast, passive S0s with positive gradients show the opposite behaviour. Furthermore, systems whose activity is dominated by star formation are structurally rounder than the rest of S0s, while those classified as Seyfert exhibit higher rotational support. The possibility that negative and positive activity gradients in S0s may result from rejuvenation by two distinct types of minor mergers is raised.
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stae097
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Accepted/In Press date: 8 January 2024
e-pub ahead of print date: 10 January 2024
Published date: 2 February 2024
Keywords:
galaxies: Seyfert, galaxies: active, galaxies: elliptical and lenticular, cD, galaxies: evolution, galaxies: star formation, galaxies: statistics
Identifiers
Local EPrints ID: 497021
URI: http://eprints.soton.ac.uk/id/eprint/497021
ISSN: 1365-2966
PURE UUID: 4f047cd2-10ef-4583-a2f1-5377d56ba628
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Date deposited: 09 Jan 2025 18:06
Last modified: 22 Aug 2025 02:45
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Contributors
Author:
J.L. Tous
Author:
J.M. Solanes
Author:
J.D. Perea
Author:
H. Domínguez-Sánchez
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