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Large-scale stellar age-velocity spiral pattern in NGC 4030

Breda, Iris; van de Ven, Glenn; Thater, Sabine; Falcón-Barroso, Jesus; Jethwa, Prashin; Gadotti, Dimitri A.; Onodera, Masato; Pessa, Ismael; Schaye, Joop; Hensler, Gerhard; Brinchmann, Jarle; Feldmeier-Krause, Anja; Krajnović, Davor; Ziegler, Bodo

Large-scale stellar age-velocity spiral pattern in NGC 4030 Thumbnail


Authors

Iris Breda

Glenn van de Ven

Sabine Thater

Jesus Falcón-Barroso

Prashin Jethwa

Masato Onodera

Ismael Pessa

Joop Schaye

Gerhard Hensler

Jarle Brinchmann

Anja Feldmeier-Krause

Davor Krajnović

Bodo Ziegler



Abstract

The processes driving the formation and evolution of late-type galaxies continue to be a debated subject in extragalactic astronomy. Investigating stellar kinematics, especially when combined with age estimates, provides crucial insights into the formation and subsequent development of galactic discs. Post-processing of exceptionally high-quality integral field spectroscopy data of NGC 4030 acquired with the Multi Unit Spectroscopic Explorer (MUSE) has revealed a striking grand design spiral pattern in the velocity dispersion map, that has not been detected in other galaxies. This pattern spatially correlates with HII regions, suggesting that stars currently being born exhibit lower velocity dispersion as compared to surrounding areas where star-formation is less active. We examined the age-velocity relation (AVR) and propose that its configuration might be shaped by a combination of heating mechanisms, seemingly consistent with findings from recent high-resolution cosmological zoom-in simulations. The complex structure of the uncovered AVR of NGC 4030 supports the hypothesis that stellar populations initially inherit the velocity dispersion σ of the progenitor cold molecular gas, which depends on formation time and galactocentric distance, subsequently experiencing kinematic heating due to cumulative gravitational interactions during their lifetime. While advancing our understanding of the AVR, these findings also offer a new framework for investigating disc heating mechanisms and their role in the evolution of galactic discs.

Citation

Breda, I., van de Ven, G., Thater, S., Falcón-Barroso, J., Jethwa, P., Gadotti, D. A., Onodera, M., Pessa, I., Schaye, J., Hensler, G., Brinchmann, J., Feldmeier-Krause, A., Krajnović, D., & Ziegler, B. (2024). Large-scale stellar age-velocity spiral pattern in NGC 4030. Astronomy & Astrophysics, 692, Article L10. https://doi.org/10.1051/0004-6361/202452595

Journal Article Type Article
Acceptance Date Nov 25, 2024
Online Publication Date Dec 17, 2024
Publication Date 2024-12
Deposit Date Jan 16, 2025
Publicly Available Date Jan 16, 2025
Journal Astronomy & Astrophysics
Print ISSN 0004-6361
Electronic ISSN 1432-0746
Publisher EDP Sciences
Peer Reviewed Peer Reviewed
Volume 692
Article Number L10
DOI https://doi.org/10.1051/0004-6361/202452595
Public URL https://durham-repository.worktribe.com/output/3337122

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