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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

Disc galaxies are still settling: Discovery of the smallest nuclear discs and their young stellar bars Thumbnail


Authors

Camila de Sá-Freitas

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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