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| Format: | Preprint |
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2025
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| Online Access: | https://arxiv.org/abs/2505.10821 |
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| _version_ | 1866915289721995264 |
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| author | Zhou, Zhimin Wang, Wenwen |
| author_facet | Zhou, Zhimin Wang, Wenwen |
| contents | To investigate the role of morphology in galaxy evolution, we analyze the relationships between galaxy structure, star formation, and HI gas content. Using multi-band images from the DESI Legacy Imaging Surveys, we perform detailed structural decompositions on a representative local galaxy sample from xGASS. Structural components and color properties are examined as functions of deviations from the star formation main sequence ($\rm ΔSFR_{MS}$) and HI gas deficiency ($\rm Δf_{HI}$). We find that bulge fractions decrease with higher $\rm ΔSFR_{MS}$ and lower stellar mass, indicating that star-forming galaxies are predominantly disc-dominated, while quiescent galaxies are bulge-dominated. The slope of the color ($g-r$) versus $\rm ΔSFR_{MS}$ relationship decreases from low to high stellar masses and from outer to inner regions, with greater color variation in massive galaxies. Color gradients are predominantly negative, becoming shallower in lower-mass galaxies and in the outer disk regions. We also identify inflection points in the color gradient and bulge fraction relations with $\rm ΔSFR_{MS}$, with main-sequence galaxies having the lowest bulge fractions and steepest color gradients. At fixed stellar mass, we observe only a slight correlation between bulge fraction and HI deficiency. However, outer disk colors show a stronger dependence on HI content than inner regions, and color gradients flatten as $\rm Δf_{HI}$ increases. These results suggest that HI gas is more closely linked to star-forming, disc-dominated systems, supporting the idea that gas accretion fuels star formation primarily in galaxy disks. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_10821 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The link between galaxy structure properties and star formation in local galaxies Zhou, Zhimin Wang, Wenwen Astrophysics of Galaxies To investigate the role of morphology in galaxy evolution, we analyze the relationships between galaxy structure, star formation, and HI gas content. Using multi-band images from the DESI Legacy Imaging Surveys, we perform detailed structural decompositions on a representative local galaxy sample from xGASS. Structural components and color properties are examined as functions of deviations from the star formation main sequence ($\rm ΔSFR_{MS}$) and HI gas deficiency ($\rm Δf_{HI}$). We find that bulge fractions decrease with higher $\rm ΔSFR_{MS}$ and lower stellar mass, indicating that star-forming galaxies are predominantly disc-dominated, while quiescent galaxies are bulge-dominated. The slope of the color ($g-r$) versus $\rm ΔSFR_{MS}$ relationship decreases from low to high stellar masses and from outer to inner regions, with greater color variation in massive galaxies. Color gradients are predominantly negative, becoming shallower in lower-mass galaxies and in the outer disk regions. We also identify inflection points in the color gradient and bulge fraction relations with $\rm ΔSFR_{MS}$, with main-sequence galaxies having the lowest bulge fractions and steepest color gradients. At fixed stellar mass, we observe only a slight correlation between bulge fraction and HI deficiency. However, outer disk colors show a stronger dependence on HI content than inner regions, and color gradients flatten as $\rm Δf_{HI}$ increases. These results suggest that HI gas is more closely linked to star-forming, disc-dominated systems, supporting the idea that gas accretion fuels star formation primarily in galaxy disks. |
| title | The link between galaxy structure properties and star formation in local galaxies |
| topic | Astrophysics of Galaxies |
| url | https://arxiv.org/abs/2505.10821 |