Stellar mass-metallicity relation throughout the large-scale structure of the Universe: CAVITY mother sample
Résumé
Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors than galaxies in denser environments, that is, in filaments, walls, and clusters. The stellar metallicity of a galaxy traces the accumulated fossil record of the star formation through the entire life of the galaxy. A comparison of the stellar metallicity of galaxies in various environments, including voids, filaments, walls, and clusters can provide valuable insights into how the large-scale environment affects the chemical evolution of the galaxy. We present the first comparison of the relation of the total stellar mass versus central stellar metallicity between galaxies in voids, filaments, walls, and clusters with different star formation history (SFH) types, morphologies, and colours for stellar masses between $10^{8.0}$ to $10^{11.5}$ solar masses and redshift $0.01
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Astrophysique [astro-ph]INSPIRE HEP : Connectez-vous pour contacter le contributeur
https://hal.science/hal-04267750
Soumis le : jeudi 2 novembre 2023-09:57:38
Dernière modification le : lundi 15 avril 2024-11:25:23
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Identifiants
- HAL Id : hal-04267750 , version 1
- ARXIV : 2310.11412
- DOI : 10.1051/0004-6361/202346884
- INSPIRE : 2711963
Citer
Jesús Domínguez-Gómez, Isabel Pérez, Tomás Ruiz-Lara, Reynier F Peletier, Patricia Sánchez-Blázquez, et al.. Stellar mass-metallicity relation throughout the large-scale structure of the Universe: CAVITY mother sample. Astronomy and Astrophysics - A&A, 2023, 680, pp.A111. ⟨10.1051/0004-6361/202346884⟩. ⟨hal-04267750⟩
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