The ALPINE-CRISTAL-JWST Survey: Chemical Abundance Comparison Between the ISM and CGM of Main-Sequence Galaxies at z=4-6
Wuji Wang, Andreas L. Faisst, Kyle Finner, Livia Vallini, Andrea Pallottini, Enrico Veraldi, Bahram Mobasher, Yu-Heng Lin, Giovanni Zamorani, Vicente Villanueva, Sylvain Veilleux, Keerthi Vasan G. C., Hannah Uebler, Akiyoshi Tsujita, Kseniia Telikova, John D. Silverman, Michael Romano, Monica Relano, Francesca Pozzi, Ambra Nanni, Juan Molina, Lun-Jun Liu, Yuan Li, Mahsa Kohandel, Anton M. Koekemoer, Hanae Inami, Edo Ibar, Rodrigo Herrera-Camus, Ali Hadi, Nicol Gutierrez-Vera, Michele Ginolfi, Seiji Fujimoto, Miroslava Dessauges-Zavadsky, Ilse De Looze, Poulomi Dam, Elisabete da Cunha, Mederic Boquien, Roberto J. Assef, Manuel Aravena, David B. Sanders
arXiv:2602.20241v1 Announce Type: new
Abstract: Gaseous halos around galaxies play an important role in galaxy evolution. The exchange of metals from the interstellar medium (ISM) to the circumgalactic medium (CGM) are caused by the formation, feedback, and/or merging history of galaxies. We study the variation in chemical composition between the ISM ($lesssim3,$kpc) and CGM ($sim5-10,$kpc) for a sample of $M_{star}>10^{9.5},M_{odot}$ main-sequence galaxies at $4arXiv:2602.20241v1 Announce Type: new
Abstract: Gaseous halos around galaxies play an important role in galaxy evolution. The exchange of metals from the interstellar medium (ISM) to the circumgalactic medium (CGM) are caused by the formation, feedback, and/or merging history of galaxies. We study the variation in chemical composition between the ISM ($lesssim3,$kpc) and CGM ($sim5-10,$kpc) for a sample of $M_{star}>10^{9.5},M_{odot}$ main-sequence galaxies at $4