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Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z = 2-4 using JWST

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00585244" target="_blank" >RIV/67985815:_____/24:00585244 - isvavai.cz</a>

  • Result on the web

    <a href="https://hdl.handle.net/11104/0353669" target="_blank" >https://hdl.handle.net/11104/0353669</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1093/mnras/stae677" target="_blank" >10.1093/mnras/stae677</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Comparing emission- and absorption-based gas-phase metallicities in GRB host galaxies at z = 2-4 using JWST

  • Original language description

    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(over dot) 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 R-23 and R-3. 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.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Monthly Notices of the Royal Astronomical Society

  • ISSN

    0035-8711

  • e-ISSN

    1365-2966

  • Volume of the periodical

    529

  • Issue of the periodical within the volume

    3

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    25

  • Pages from-to

    2807-2831

  • UT code for WoS article

    001188770300012

  • EID of the result in the Scopus database

    2-s2.0-85188705507