GA-NIFS: A smouldering disk galaxy undergoing ordered rotation at z=4.26
Fuente:
arXiv
Saved in:
| Main Authors: | , , , , , , , , , , , , , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866911302477152256 |
|---|---|
| author | Jones, Gareth C. Maiolino, Roberto D'Eugenio, Francesco Arribas, Santiago Bunker, Andrew J. Charlot, Stephane Perna, Michele del Pino, Bruno Rodriguez Übler, Hannah Böker, Torsten Cresci, Giovanni Lamperti, Isabella Parlanti, Eleonora Pascalau, Robert Scholtz, Jan Zamora, Sandra |
| author_facet | Jones, Gareth C. Maiolino, Roberto D'Eugenio, Francesco Arribas, Santiago Bunker, Andrew J. Charlot, Stephane Perna, Michele del Pino, Bruno Rodriguez Übler, Hannah Böker, Torsten Cresci, Giovanni Lamperti, Isabella Parlanti, Eleonora Pascalau, Robert Scholtz, Jan Zamora, Sandra |
| contents | Rotating galaxies with relaxed gaseous disks have been discovered across cosmic time, from the local Universe to high redshift (z>4). But few such sources have been confirmed at z>4, making them a precious sample to examine what conditions result in such ordered kinematics in an early, more chaotic Universe. One of the best examples of this sample is the galaxy DLA0817g1 (z=4.2603), which shows remarkably clear rotation in ALMA [CII] data. We present recent JWST/NIRSpec IFU data (R~2700) of DLA0817g1, which we combine with archival ALMA [CII] observations to place constraints on its ISM conditions and morpho-kinematics. From a combination of line ratios, we find a high gas-phase metallicity (~0.7 solar), high fraction of obscured star formation, low ionisation (compared to other high-redshift galaxies observed with JWST), and no significant evidence for AGN (based on the WHAN diagnostic). Dynamical modelling with 3DBarolo reveal nearly identical rotation in Halpha and [CII], but with a higher velocity dispersion in the former. Using our metallicity estimate and previous CO and [CII] detections, we derive a new estimate of the molecular gas mass, relieving a previous strain in the mass budget. Altogether, we suggest that this is a 'smouldering' galaxy, where past star formation resulted in significant chemical enrichment (i.e., Zgas and Mdust), but the current activity is low (i.e., lower ionisation parameter and electron temperature). These new observations have opened a window into questions regarding the interplay of gas, metallicity, star formation, and kinematics in a prototypical early disk galaxy. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2512_05213 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | GA-NIFS: A smouldering disk galaxy undergoing ordered rotation at z=4.26 Jones, Gareth C. Maiolino, Roberto D'Eugenio, Francesco Arribas, Santiago Bunker, Andrew J. Charlot, Stephane Perna, Michele del Pino, Bruno Rodriguez Übler, Hannah Böker, Torsten Cresci, Giovanni Lamperti, Isabella Parlanti, Eleonora Pascalau, Robert Scholtz, Jan Zamora, Sandra Astrophysics of Galaxies Rotating galaxies with relaxed gaseous disks have been discovered across cosmic time, from the local Universe to high redshift (z>4). But few such sources have been confirmed at z>4, making them a precious sample to examine what conditions result in such ordered kinematics in an early, more chaotic Universe. One of the best examples of this sample is the galaxy DLA0817g1 (z=4.2603), which shows remarkably clear rotation in ALMA [CII] data. We present recent JWST/NIRSpec IFU data (R~2700) of DLA0817g1, which we combine with archival ALMA [CII] observations to place constraints on its ISM conditions and morpho-kinematics. From a combination of line ratios, we find a high gas-phase metallicity (~0.7 solar), high fraction of obscured star formation, low ionisation (compared to other high-redshift galaxies observed with JWST), and no significant evidence for AGN (based on the WHAN diagnostic). Dynamical modelling with 3DBarolo reveal nearly identical rotation in Halpha and [CII], but with a higher velocity dispersion in the former. Using our metallicity estimate and previous CO and [CII] detections, we derive a new estimate of the molecular gas mass, relieving a previous strain in the mass budget. Altogether, we suggest that this is a 'smouldering' galaxy, where past star formation resulted in significant chemical enrichment (i.e., Zgas and Mdust), but the current activity is low (i.e., lower ionisation parameter and electron temperature). These new observations have opened a window into questions regarding the interplay of gas, metallicity, star formation, and kinematics in a prototypical early disk galaxy. |
| title | GA-NIFS: A smouldering disk galaxy undergoing ordered rotation at z=4.26 |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2512.05213 |