Camila de Sá-Freitas
Disc galaxies are still settling: Discovery of the smallest nuclear discs and their young stellar bars
de Sá-Freitas, Camila; Gadotti, Dimitri A.; Fragkoudi, Francesca; Coccato, Lodovico; Coelho, Paula; de Lorenzo-Cáceres, Adriana; Falcón-Barroso, Jesús; Kolcu, Tutku; Martín-Navarro, Ignacio; Mendez-Abreu, Jairo; Neumann, Justus; Blazquez, Patricia Sanchez; Querejeta, Miguel; van de Ven, Glenn
Authors
Dr Dimitri Gadotti dimitri.a.gadotti@durham.ac.uk
Assistant Professor
Dr Francesca Fragkoudi francesca.fragkoudi@durham.ac.uk
Assistant Professor
Lodovico Coccato
Paula Coelho
Adriana de Lorenzo-Cáceres
Jesús Falcón-Barroso
Tutku Kolcu
Ignacio Martín-Navarro
Jairo Mendez-Abreu
Justus Neumann
Patricia Sanchez Blazquez
Miguel Querejeta
Glenn van de Ven
Abstract
When galactic discs settle and become massive enough, they are able to form stellar bars. These non-axisymmetric structures induce shocks in the gas, causing it to flow to the centre where nuclear structures, such as nuclear discs and rings, are formed. Previous theoretical and observational studies have hinted at the co-evolution of bars and nuclear discs, suggesting that nuclear discs grow ‘inside-out’ and thereby proposing that smaller discs reside in younger bars. Nevertheless, it remains unclear how the bar and the nuclear structures form and evolve over time. The smallest nuclear discs discovered to date tend to be larger than ∼200 pc, even though some theoretical studies have reported that when nuclear discs form, they can be much smaller. Using MUSE archival data, we report, for the first time, two extragalactic nuclear discs with radius measurements below 100 pc. Additionally, our estimations reveal the youngest bars found to date. We estimate that the bars in these galaxies formed 4.50−1.10+1.60(sys)−0.75+1.00(stat) and 0.7+2.60(sys)−0.05+0.05(stat) Gyr ago, for NGC 289 and NGC 1566, respectively. This suggests that at least some disc galaxies in the Local Universe may still be dynamically settling. By adding these results to previous findings in the literature, we are able to retrieve a stronger correlation between nuclear disc size and bar length. We also derive a tentative exponential growth scenario for nuclear discs.
Citation
de Sá-Freitas, C., Gadotti, D. A., Fragkoudi, F., Coccato, L., Coelho, P., de Lorenzo-Cáceres, A., …van de Ven, G. (2023). Disc galaxies are still settling: Discovery of the smallest nuclear discs and their young stellar bars. Astronomy & Astrophysics, 678, Article A202. https://doi.org/10.1051/0004-6361/202347028
Journal Article Type | Article |
---|---|
Acceptance Date | Aug 4, 2023 |
Online Publication Date | Oct 24, 2023 |
Publication Date | 2023-10 |
Deposit Date | Jan 22, 2024 |
Publicly Available Date | Jan 22, 2024 |
Journal | Astronomy & Astrophysics |
Print ISSN | 0004-6361 |
Electronic ISSN | 1432-0746 |
Publisher | EDP Sciences |
Peer Reviewed | Peer Reviewed |
Volume | 678 |
Article Number | A202 |
DOI | https://doi.org/10.1051/0004-6361/202347028 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://durham-repository.worktribe.com/output/2160953 |
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Copyright Statement
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0).
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