Growing a nuclear star cluster from star formation and cluster mergers: The JWST NIRSpec view of NGC 4654
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| Autores principales: | , , , , , , , , , , , , |
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| Formato: | Preprint |
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2024
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| _version_ | 1866914856323514368 |
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| author | Fahrion, Katja Böker, Torsten Perna, Michele Beck, Tracy L. Maiolino, Roberto Arribas, Santiago Bunker, Andrew J. Charlot, Stephane Ceci, Matteo Cresci, Giovanni De Marchi, Guido Lützgendorf, Nora Ulivi, Lorenzo |
| author_facet | Fahrion, Katja Böker, Torsten Perna, Michele Beck, Tracy L. Maiolino, Roberto Arribas, Santiago Bunker, Andrew J. Charlot, Stephane Ceci, Matteo Cresci, Giovanni De Marchi, Guido Lützgendorf, Nora Ulivi, Lorenzo |
| contents | We present a detailed study of the centre of NGC4654, a Milky Way-like spiral galaxy in the Virgo cluster that has been reported to host a double stellar nucleus, thus promising a rare view of ongoing star cluster infall into a galaxy nucleus. Analysing JWST NIRSpec integral-field spectroscopic data and Hubble Space Telescope imaging of the inner 330 $\times$ 330 pc, we find that the nucleus harbours in fact three massive star clusters. Maps of infrared emission lines from NIRSpec show different morphologies for the ionised and molecular gas components. The emission from molecular hydrogen gas is concentrated at the NSC location, while emission from hydrogen recombination lines is more extended beyond the central cluster. The velocity fields of both gas and stars indicate that the three clusters are part of a complicated dynamical system, with the NSC having an elevated velocity dispersion in line with its high stellar mass. To investigate the stellar populations of the three clusters in more detail, we use surface brightness modelling to measure their fluxes from ultraviolet to mid-infrared wavelengths and fit their spectral energy distributions (SEDs). Two of the clusters are UV-bright and well described by single stellar populations with young ages ($\sim$ 3 and 5 Myr) and low masses ($M_\ast \sim 4 \times 10^{4} - 10^{5} M_\odot$), whereas the central cluster is much more massive ($3 \times 10^7 M_\odot$), and cannot be fitted by a single stellar population. Instead, we find that a minor young population ($\sim$ 1 Myr) embedded in a dominant old population ($\sim$ 8 Gyr) is needed to explain its SED. Given its complex composition and the close proximity of two young star clusters that are likely to merge with it within a few hundred million years, we consider NGC4654 a unique laboratory to study NSC growth from both in-situ star formation and the infall of star clusters. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_08910 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Growing a nuclear star cluster from star formation and cluster mergers: The JWST NIRSpec view of NGC 4654 Fahrion, Katja Böker, Torsten Perna, Michele Beck, Tracy L. Maiolino, Roberto Arribas, Santiago Bunker, Andrew J. Charlot, Stephane Ceci, Matteo Cresci, Giovanni De Marchi, Guido Lützgendorf, Nora Ulivi, Lorenzo Astrophysics of Galaxies We present a detailed study of the centre of NGC4654, a Milky Way-like spiral galaxy in the Virgo cluster that has been reported to host a double stellar nucleus, thus promising a rare view of ongoing star cluster infall into a galaxy nucleus. Analysing JWST NIRSpec integral-field spectroscopic data and Hubble Space Telescope imaging of the inner 330 $\times$ 330 pc, we find that the nucleus harbours in fact three massive star clusters. Maps of infrared emission lines from NIRSpec show different morphologies for the ionised and molecular gas components. The emission from molecular hydrogen gas is concentrated at the NSC location, while emission from hydrogen recombination lines is more extended beyond the central cluster. The velocity fields of both gas and stars indicate that the three clusters are part of a complicated dynamical system, with the NSC having an elevated velocity dispersion in line with its high stellar mass. To investigate the stellar populations of the three clusters in more detail, we use surface brightness modelling to measure their fluxes from ultraviolet to mid-infrared wavelengths and fit their spectral energy distributions (SEDs). Two of the clusters are UV-bright and well described by single stellar populations with young ages ($\sim$ 3 and 5 Myr) and low masses ($M_\ast \sim 4 \times 10^{4} - 10^{5} M_\odot$), whereas the central cluster is much more massive ($3 \times 10^7 M_\odot$), and cannot be fitted by a single stellar population. Instead, we find that a minor young population ($\sim$ 1 Myr) embedded in a dominant old population ($\sim$ 8 Gyr) is needed to explain its SED. Given its complex composition and the close proximity of two young star clusters that are likely to merge with it within a few hundred million years, we consider NGC4654 a unique laboratory to study NSC growth from both in-situ star formation and the infall of star clusters. |
| title | Growing a nuclear star cluster from star formation and cluster mergers: The JWST NIRSpec view of NGC 4654 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2404.08910 |