GA-NIFS: An extremely nitrogen-loud and chemically stratified galaxy at $z\sim 5.55$
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| Natura: | Preprint |
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2024
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| author | Ji, Xihan Übler, Hannah Maiolino, Roberto D'Eugenio, Francesco Arribas, Santiago Bunker, Andrew J. Charlot, Stéphane Perna, Michele Del Pino, Bruno Rodríguez Böker, Torsten Cresci, Giovanni Curti, Mirko Kumari, Nimisha Lamperti, Isabella |
| author_facet | Ji, Xihan Übler, Hannah Maiolino, Roberto D'Eugenio, Francesco Arribas, Santiago Bunker, Andrew J. Charlot, Stéphane Perna, Michele Del Pino, Bruno Rodríguez Böker, Torsten Cresci, Giovanni Curti, Mirko Kumari, Nimisha Lamperti, Isabella |
| contents | We report the chemical abundance pattern of GS\_3073, a galaxy at $z=5.55$ which was previously confirmed to host an overmassive active black hole, by leveraging the detection of about 40 emission lines, combining JWST/NIRSpec observations and ground-based (VLT/VIMOS) data. Based on the rest-frame UV emission lines, which trace high-density ($\sim 10^5~{\rm cm}^{-3}$) and highly ionized gas, we derived an abundance ratio of $\rm log(N/O) = 0.42^{+0.13}_{-0.10}$. At an estimated metallicity of $0.2~Z_{\odot}$, this is the most extreme nitrogen-rich object found by JWST thus far. In comparison, the relative carbon abundance derived from the rest-frame UV emission lines is $\rm log(C/O) = -0.38^{+0.13}_{-0.11}$, which is not significantly higher than those in local galaxies and stars with similar metallicities. We also found potential detection of coronal lines including [FeVII]$λ6087$ and [FeXIV]$λ5303$, both blended with [CaV]. We inferred a range of Fe abundances compatible with those in local stars and galaxies. Overall, the chemical abundance pattern of GS\_3073 is compatible with enrichment by super-massive stars with $M_* \gtrsim 1000~M_\odot$, asymptotic giant branch (AGB) stars, or Wolf-Rayet (WR) stars. Interestingly, when using optical emission lines which trace lower density ($\sim 10^3~{\rm cm}^{-3}$) and lower ionization gas, we found a sub-solar N/O ratio. We interpret the difference in N/O derived from UV lines and optical lines as evidence for a stratified system, where the inner and denser region is both more chemically enriched and more ionized. Taking this luminous, well-studied system as a benchmark, our results suggest that nitrogen loudness in high-$z$ galaxies is confined to the central, dense, and highly ionized region of the galaxies, while the bulk of the galaxies evolves more normally. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2404_04148 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | GA-NIFS: An extremely nitrogen-loud and chemically stratified galaxy at $z\sim 5.55$ Ji, Xihan Übler, Hannah Maiolino, Roberto D'Eugenio, Francesco Arribas, Santiago Bunker, Andrew J. Charlot, Stéphane Perna, Michele Del Pino, Bruno Rodríguez Böker, Torsten Cresci, Giovanni Curti, Mirko Kumari, Nimisha Lamperti, Isabella Astrophysics of Galaxies We report the chemical abundance pattern of GS\_3073, a galaxy at $z=5.55$ which was previously confirmed to host an overmassive active black hole, by leveraging the detection of about 40 emission lines, combining JWST/NIRSpec observations and ground-based (VLT/VIMOS) data. Based on the rest-frame UV emission lines, which trace high-density ($\sim 10^5~{\rm cm}^{-3}$) and highly ionized gas, we derived an abundance ratio of $\rm log(N/O) = 0.42^{+0.13}_{-0.10}$. At an estimated metallicity of $0.2~Z_{\odot}$, this is the most extreme nitrogen-rich object found by JWST thus far. In comparison, the relative carbon abundance derived from the rest-frame UV emission lines is $\rm log(C/O) = -0.38^{+0.13}_{-0.11}$, which is not significantly higher than those in local galaxies and stars with similar metallicities. We also found potential detection of coronal lines including [FeVII]$λ6087$ and [FeXIV]$λ5303$, both blended with [CaV]. We inferred a range of Fe abundances compatible with those in local stars and galaxies. Overall, the chemical abundance pattern of GS\_3073 is compatible with enrichment by super-massive stars with $M_* \gtrsim 1000~M_\odot$, asymptotic giant branch (AGB) stars, or Wolf-Rayet (WR) stars. Interestingly, when using optical emission lines which trace lower density ($\sim 10^3~{\rm cm}^{-3}$) and lower ionization gas, we found a sub-solar N/O ratio. We interpret the difference in N/O derived from UV lines and optical lines as evidence for a stratified system, where the inner and denser region is both more chemically enriched and more ionized. Taking this luminous, well-studied system as a benchmark, our results suggest that nitrogen loudness in high-$z$ galaxies is confined to the central, dense, and highly ionized region of the galaxies, while the bulk of the galaxies evolves more normally. |
| title | GA-NIFS: An extremely nitrogen-loud and chemically stratified galaxy at $z\sim 5.55$ |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2404.04148 |