Put a ring on it: the origin of star-forming rings in S0 galaxies
Creators: name: Tous, José Luis
name: Perea, Jaime
name: Solanes, José Maria
name: Domínguez-Sánchez, Helena
Publisher: name: Zenodo
Year: 2022
Subjects: Lenticular galaxies
Galaxy spectroscopy
Galaxy structure
Galaxy evolution

description: The examination of the spatially resolved IFS maps in a sample of more than 500 lenticular (S0) galaxies drawn from the MaNGA survey has unveiled the existence of transient inner annular structures (〈R〉 ∼ 1 R<sub>e</sub>) betraying ongoing star formation in a good number of these objects. Activity gradients in these galaxies have been measured through a novel methodology based on the principal component analysis of their optical spectra averaged over bins of galactocentric radius. We find that the sign of these gradients is closely linked to the presence of rings in the spectral maps, which are specially conspicuous in the equivalent width of Hα-emission, EW(Hα), with a fractional abundance —22–37% depending on the strictness of ring identification— larger than that inferred from optical imaging. While the numbers of S0s with globally positive, negative, and flat activity gradients are comparable, star-forming rings are found almost exclusively in objects with a positive slope for which quenching proceeds inside-out, in good agreement with predictions from cosmological simulations studying S0 buildup. The assessment of these structures and the properties of the galaxies harboring them also indicates that the frequency of such rings increases with the mass of their hosts, that they feed mainly on the gas from the disks, that are more short-lived in galaxies with ongoing star formation, and that the local environment does not play a relevant role in their formation. From the present analysis, we conclude that the presence of rings in the EW of the Hα emission line is a common phenomenon among fully formed S0s, possibly associated with annular disk resonances driven by weakly disruptive mergers preferentially involving the more massive representatives of these galaxies and their smaller and closer satellites.
description: We acknowledge financial support from the Spanish state agency MCIN/AEI/10.13039/501100011033 and by 'ERDF A way of making Europe' funds through research grants PID2019–106027GB–C41 and PID2019–106027GB–C43. MCIN/AEI/10.13039/501100011033758 has also provided additional support through the Centre of Excellence Severo Ochoa's award for the Instituto de Astrofísica de Andalucía under contract SEV–2017–0709 and the Centre of Excellence María de Maeztu's award for the Institut de Ciències del Cosmos at the Universitat de Barcelona under contract CEX2019–000918–M. J.L.T. acknowledges support by the PRE2020–091838 grant from MCIN/AEI/10.13039/501100011033766 and by 'FSE Invests in your future'. H.D.S. acknowledges support by the PID2020-115098RJ-I00 grant from MCIN/AEI/10.13039/501100011033.
description: {"references": ["Deeley, S., Drinkwater, M. J., Sweet, S. M., et al. 2021, MNRAS, 508, 895, 2021MNRAS.508..895D", "Jim\u00e9nez-Palau, C., Solanes, J. M., Perea, J. D., del Olmo A., &amp; Tous, J. L. 2022, MNRAS, 515, 3956, 2022MNRAS.515.3956J", "Mapelli, M., Rampazzo, R., &amp; Marino, A. 2015, A&amp;A, 575, A16, 2015A&amp;A...575A..16M", "Tous, J. L., Solanes, J. M., &amp; Perea, J. D. 2020, MNRAS, 495, 4135, 2020MNRAS.495.4135T"]}