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Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z =2-4 using JWST
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Number of Authors: 372024 (English)In: Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, E-ISSN 1365-2966, Vol. 529, no 3, p. 2807-2831Article in journal (Refereed) Published
Abstract [en]

Much of what is known of the chemical composition of the universe is based on emission line spectra from star-forming galaxies. Emission-based inferences are, nevertheless, model-dependent and they are dominated by light from luminous star-forming regions. An alternative and sensitive probe of the metallicity of galaxies is through absorption lines imprinted on the luminous afterglow spectra of long gamma ray bursts (GRBs) from neutral material within their host galaxy. We present results from a JWST/NIRSpec programme to investigate for the first time the relation between the metallicity of neutral gas probed in absorption by GRB afterglows and the metallicity of the star-forming regions for the same host galaxy sample. Using an initial sample of eight GRB host galaxies at z = 2.1–4.7, we find a tight relation between absorption and emission line metallicities when using the recently proposed 𝑅^ metallicity diagnostic (±0.2 dex). This agreement implies a relatively chemically homogeneous multiphase interstellar medium and indicates that absorption and emission line probes can be directly compared. However, the relation is less clear when using other diagnostics, such as R23 and R3. We also find possible evidence of an elevated N/O ratio in the host galaxy of GRB 090323 at z = 4.7, consistent with what has been seen in other z > 4 galaxies. Ultimate confirmation of an enhanced N/O ratio and of the relation between absorption and emission line metallicities will require a more direct determination of the emission line metallicity via the detection of temperature-sensitive auroral lines in our GRB host galaxy sample.

Place, publisher, year, edition, pages
2024. Vol. 529, no 3, p. 2807-2831
Keywords [en]
gamma-ray burst: general, ISM: abundances, galaxies: abundances, galaxies: high-redshift, galaxies: ISM, quasars: absorption lines
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:su:diva-228652DOI: 10.1093/mnras/stae677ISI: 001188770300012Scopus ID: 2-s2.0-85188705507OAI: oai:DiVA.org:su-228652DiVA, id: diva2:1854565
Available from: 2024-04-26 Created: 2024-04-26 Last updated: 2024-04-26Bibliographically approved

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Schulze, Steve

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Schady, P.Yates, R. M.Rossi, A.Schulze, SteveWiseman, P.
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The Oskar Klein Centre for Cosmo Particle Physics (OKC)Department of Physics
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Monthly notices of the Royal Astronomical Society
Astronomy, Astrophysics and Cosmology

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