2023ApJ...951L..17J


Query : 2023ApJ...951L..17J

2023ApJ...951L..17J - Astrophys. J., 951, L17 (2023/July-1)

Early Results from GLASS-JWST. XXI. Rapid Asembly of a Galaxy at z = 6.23 Revealed by Its C/O Abundance.

JONES T., SANDERS R., CHEN Y., WANG X., MORISHITA T., ROBERTS-BORSANI G., TREU T., DRESSLER A., MERLIN E., PARIS D., SANTINI P., BERGAMINI P., HENRY A., HUNTZINGER E., NANAYAKKARA T., BOYETT K., BRADAC M., BRAMMER G., CALABRO A., GLAZEBROOK K., GRASHA K., MASCIA S., PENTERICCI L., TRENTI M. and VULCANI B.

Abstract (from CDS):

The abundance of carbon relative to oxygen (C/O) is a promising probe of star formation history in the early universe, as the ratio changes with time due to production of these elements by different nucleosynthesis pathways. We present a measurement of $\mathrm{log}({\rm{C}}/{\rm{O}})=-1.01\pm 0.12$ (stat) ±0.15 (sys) in a z = 6.23 galaxy observed as part of the GLASS-JWST Early Release Science Program. Notably, we achieve good precision thanks to the detection of the rest-frame ultraviolet O III], C III], and C IV emission lines delivered by JWST/NIRSpec. The C/O abundance is ∼0.8 dex lower than the solar value and is consistent with the expected yield from core-collapse supernovae, indicating that longer-lived intermediate-mass stars have not fully contributed to carbon enrichment. This in turn implies rapid buildup of a young stellar population with age ≲100 Myr in a galaxy seen ∼900 Myr after the big bang. Our chemical abundance analysis is consistent with spectral energy distribution modeling of JWST/NIRCam photometric data, which indicates a current stellar mass $\mathrm{log}\,{M}_{* }/{M}_{\odot }={8.4}_{-0.2}^{+0.4}$ and specific star formation rate ≃20 Gyr–1. These results showcase the value of chemical abundances and C/O in particular to study the earliest stages of galaxy assembly.

Abstract Copyright: © 2023. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): High-redshift galaxies - Galaxy abundances - Abundance ratios - Emission line galaxies

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 [MPC2023] GLASS 150008 LeG 00 14 24.607 -30 25 09.24           ~ 21 0

Query : 2023ApJ...951L..17J

Basic data :
[MPC2023] GLASS 150008 -- Gravitationally Lensed Image of a Galaxy
Other object types:
otypes_help
LeG (2023A&A,[MPC2023]), G (2023ApJ)
ICRS coord. (ep=J2000) :
00 14 24.607 -30 25 09.24 (Near-IR) [ ] C 2023ApJ...951L..17J
FK4 coord. (ep=B1950 eq=1950) :
00 11 53.105 -30 41 50.04 [ ]
Gal coord. (ep=J2000) :
008.668328 -81.247897 [ ]
Radial velocity / Redshift / cz :
V(km/s) 288534 [21] / z(spectroscopic) 6.22895 [0.00007] / cz 1867392.2 [21.0]
   (NIR) D 2023ApJ...951L..17J
Fluxes (1) :
F150W 25.8 [~] D 2023A&A...672A.155M
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[MPC2023] GLASS 150008

References (21 between 1850 and 2026) (Total 21)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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