The GECKOS survey: Jeans anisotropic models of edge-on discs uncover the impact of dust and kinematic structures

Rutherford, TH, Fraser-McKelvie, A, Emsellem, E, van de Sande, J, Croom, SM, Poci, A, Martig, M ORCID: 0000-0001-5454-1492, Gadotti, DA, Pinna, F, Valenzuela, LM, van de Ven, G, Bland-Hawthorn, J, Das, P, Davis, TA, Elliott, R, Fisher, DB, Hayden, MR, Mailvaganam, A, Sharma, S and Zafar, T The GECKOS survey: Jeans anisotropic models of edge-on discs uncover the impact of dust and kinematic structures. Astronomy & Astrophysics. ISSN 0004-6361 (Accepted)

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Abstract

The central regions of disc galaxies host a rich variety of stellar structures: nuclear discs, bars, bulges, and boxy-peanut bulges. These components are often difficult to disentangle, both photometrically and kinematically, particularly in star-forming galaxies where dust obscuration and complex stellar motions complicate interpretation. In this work, we used data from the GECKOS-MUSE survey to investigate the impact of dust on axisymmetric Jeans Anisotropic Multi-Gaussian Expansion (JAM) models and assess their ability to recover kinematic structures in edge-on disc galaxies. We constructed JAM models for a sample of seven edge-on (i ⪆ 85^̧irc) galaxies that span a range of star formation rates, dust content, and kinematic complexity. We find that when dust is appropriately masked, the disc regions of each galaxy are fit to ̧hi^2_ reduced łeq 5. We analysed 2D residual velocity fields to identify signatures of non-axisymmetric structure. We find that derived dynamical masses are constant within 10% for each galaxy across all dust masking levels. In NGC,3957, a barred boxy galaxy in our sample, we identified velocity residuals that persist even under aggressive dust masking, aligned with bar orbits and supported by photometric bar signatures. We extended this analysis to reveal a bar in IC,1711 and a possible side-on bar in NGC,0522. Our results highlight both the capabilities and limitations of JAM in dusty, edge-on systems and attempt to link residual velocities to known non-axisymmetric kinematic structure.

Item Type:	Article
Uncontrolled Keywords:	5109 Space Sciences; 51 Physical Sciences; 0201 Astronomical and Space Sciences; Astronomy & Astrophysics; 5101 Astronomical sciences; 5107 Particle and high energy physics; 5109 Space sciences
Subjects:	Q Science > QB Astronomy Q Science > QC Physics
Divisions:	Astrophysics Research Institute
Publisher:	EDP Sciences
Date of acceptance:	9 September 2025
Date of first compliant Open Access:	6 November 2025
Date Deposited:	06 Nov 2025 15:39
Last Modified:	06 Nov 2025 16:00
DOI or ID number:	10.1051/0004-6361/202556418
URI:	https://researchonline.ljmu.ac.uk/id/eprint/27513

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