Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster II. Stellar kinematics and dynamical masses
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| Format: | Preprint |
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2025
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| author | Buttitta, Chiara Iodice, Enrichetta Doll, Goran Hartke, Johanna Hilker, Michael Forbes, Duncan A. Corsini, Enrico M. Rossi, Luca Arnaboldi, Magda Cantiello, Michele D'Ago, Giuseppe Falcon-Barroso, Jesus Gullieuszik, Marco La Marca, Antonio Mieske, Steffen Mirabile, Marco Paolillo, Maurizio Rejkuba, Marina Spavone, Marilena Spiniello, Chiara Sarzi, Marc |
| author_facet | Buttitta, Chiara Iodice, Enrichetta Doll, Goran Hartke, Johanna Hilker, Michael Forbes, Duncan A. Corsini, Enrico M. Rossi, Luca Arnaboldi, Magda Cantiello, Michele D'Ago, Giuseppe Falcon-Barroso, Jesus Gullieuszik, Marco La Marca, Antonio Mieske, Steffen Mirabile, Marco Paolillo, Maurizio Rejkuba, Marina Spavone, Marilena Spiniello, Chiara Sarzi, Marc |
| contents | Context: This paper focuses on a class of galaxies characterised by an extremely low surface brightness: the ultra-diffuse galaxies (UDGs). We used new integral-field spectroscopic data from the ESO Large Programme Looking into the faintEst WIth MUSE (LEWIS) project. Aims: Our main goals are addressing the formation channels and investigating possible correlations of their observational properties. In particular, we derive their stellar kinematics and dynamical properties. Methods: We extract the 1D stacked spectrum inside the effective radius to obtain an unbiased measure of $σ_{\rm eff}$. To derive the spatially-resolved stellar kinematics, we first apply the Voronoi tessellation algorithm to bin the spaxels in the datacube and then follow the same prescription adopted for the 1D case. In addition, we extract the velocity profiles along the galaxy's major and minor axes. Results: We find that 7 out of 18 UDGs in LEWIS show a mild rotation, 5 do not have evidence of any rotation, and the remaining 6 UDGs are unconstrained cases. This is the first large census of velocity profiles for UDGs. On average, UDGs in LEWIS are characterised by low values of $σ_{\rm eff}$, comparable with available values from the literature. In the Faber-Jackson relation plane, we found a group of UDGs consistent with the relation within the errorbars, whereas outliers are objects with non-negligible rotation components. UDGs and LSBs in LEWIS have larger dark matter content than dwarf galaxies with similar total luminosity. We do not find clear correlations between the derived properties and the local environment. Conclusions: Based on the stellar kinematics, two classes of UDGs are found in the Hydra I cluster: the rotating and non-rotating systems. This result, combined with other structural properties, can help to discriminate between the several formation scenarios proposed for UDGs. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2501_16190 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster II. Stellar kinematics and dynamical masses Buttitta, Chiara Iodice, Enrichetta Doll, Goran Hartke, Johanna Hilker, Michael Forbes, Duncan A. Corsini, Enrico M. Rossi, Luca Arnaboldi, Magda Cantiello, Michele D'Ago, Giuseppe Falcon-Barroso, Jesus Gullieuszik, Marco La Marca, Antonio Mieske, Steffen Mirabile, Marco Paolillo, Maurizio Rejkuba, Marina Spavone, Marilena Spiniello, Chiara Sarzi, Marc Astrophysics of Galaxies Context: This paper focuses on a class of galaxies characterised by an extremely low surface brightness: the ultra-diffuse galaxies (UDGs). We used new integral-field spectroscopic data from the ESO Large Programme Looking into the faintEst WIth MUSE (LEWIS) project. Aims: Our main goals are addressing the formation channels and investigating possible correlations of their observational properties. In particular, we derive their stellar kinematics and dynamical properties. Methods: We extract the 1D stacked spectrum inside the effective radius to obtain an unbiased measure of $σ_{\rm eff}$. To derive the spatially-resolved stellar kinematics, we first apply the Voronoi tessellation algorithm to bin the spaxels in the datacube and then follow the same prescription adopted for the 1D case. In addition, we extract the velocity profiles along the galaxy's major and minor axes. Results: We find that 7 out of 18 UDGs in LEWIS show a mild rotation, 5 do not have evidence of any rotation, and the remaining 6 UDGs are unconstrained cases. This is the first large census of velocity profiles for UDGs. On average, UDGs in LEWIS are characterised by low values of $σ_{\rm eff}$, comparable with available values from the literature. In the Faber-Jackson relation plane, we found a group of UDGs consistent with the relation within the errorbars, whereas outliers are objects with non-negligible rotation components. UDGs and LSBs in LEWIS have larger dark matter content than dwarf galaxies with similar total luminosity. We do not find clear correlations between the derived properties and the local environment. Conclusions: Based on the stellar kinematics, two classes of UDGs are found in the Hydra I cluster: the rotating and non-rotating systems. This result, combined with other structural properties, can help to discriminate between the several formation scenarios proposed for UDGs. |
| title | Looking into the faintEst WIth MUSE (LEWIS): Exploring the nature of ultra-diffuse galaxies in the Hydra-I cluster II. Stellar kinematics and dynamical masses |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2501.16190 |