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    Please use this identifier to cite or link to this item: https://tkuir.lib.tku.edu.tw/dspace/handle/987654321/125543


    Title: The metallicity's fundamental dependence on both local and global galactic quantities
    Authors: William M. Baker, Roberto Maiolino, Francesco Belfiore, Mirko Curti, Asa F. L. Bluck, Lihwai Lin, Sara L. Ellison, Mallory Thorp, Hsi-An Pan
    Keywords: galaxies: abundances, galaxies: evolution, galaxies: general, galaxies: ISM
    Date: 2023-02
    Issue Date: 2024-07-23 12:05:28 (UTC+8)
    Publisher: Oxford University Press
    Abstract: We study the scaling relations between gas-phase metallicity, stellar mass surface density (Σ*), star formation rate surface density (ΣSFR), and molecular gas surface density (⁠
    ⁠) in local star-forming galaxies on scales of a kpc. We employ optical integral field spectroscopy from the Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, and ALMA data for a subset of MaNGA galaxies. We use partial correlation coefficients and Random Forest regression to determine the relative importance of local and global galactic properties in setting the gas-phase metallicity. We find that the local metallicity depends primarily on Σ* (the resolved mass–metallicity relation, rMZR), and has a secondary anticorrelation with ΣSFR (i.e. a spatially resolved version of the ‘Fundamental Metallicity Relation’, rFMR). We find that
    is less important than ΣSFR in determining the local metallicity. This result indicates that gas accretion, resulting in local metallicity dilution and local boosting of star formation, is unlikely to be the primary origin of the rFMR. The local metallicity depends also on the global properties of galaxies. We find a strong dependence on the total stellar mass (M*) and a weaker (inverse) dependence on the total SFR. The global metallicity scaling relations, therefore, do not simply stem out of their resolved counterparts; global properties and processes, such as the global gravitational potential well, galaxy-scale winds and global redistribution/mixing of metals, likely contribute to the local metallicity, in addition to local production and retention.
    Relation: Monthly Notices of the Royal Astronomical Society 519(1), pp.1149-1170
    DOI: 10.1093/mnras/stac3594
    Appears in Collections:[物理學系暨研究所] 期刊論文

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