CEERS: Forging the First Dust -- Transition from Stellar to ISM Grain Growth in the Early Universe

CEERS: Forging the First Dust -- Transition from Stellar to ISM Grain Growth in the Early Universe

We investigate the coevolution of metals and dust for 173 galaxies at 4.08 presents a metal-to-stellar mass ratio larger than a few 10^-3, above a floor. This suggests a very fast rise of metals at high redshift, impacting the tentative detections of population III objects.

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Bibliographische Detailangaben
Hauptverfasser: Burgarella, Denis, Buat, Véronique, Theulé, Patrice, Zavala, Jorge, Haro, Pablo Arrabal, Bagley, Micaela B, Boquien, Médéric, Cleri, Nikko, Dewachter, Tim, Dickinson, Mark, Ferguson, Henry C, Fernández, Vital, Finkelstein, Steven L, Fontana, Adriano, Gawiser, Eric, Grazian, Andrea, Grogin, Norman, Holwerda, Benne W, Kartaltepe, Jeyhan S, Kewley, Lisa, Kirkpatrick, Allison, Kocevski, Dale, Koekemoer, Anton M, Long, Arianna, Lotz, Jennifer, Lucas, Ray A, Mobasher, Bahram, Papovich, Casey, Pérez-González, Pablo G, Pirzkal, Nor, Ravindranath, Swara, Rodighiero, Giulia, Roehlly, Yannick, Rose, Caitlin, Seillé, Lise-Marie, Somerville, Rachel, Wilkins, Steve, Yang, Guang, Yung, L. Y. Aaron
Format: Artikel
Sprache:eng
Schlagworte:
Physics - Astrophysics of Galaxies
Physics - Cosmology and Nongalactic Astrophysics
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Beschreibung
Zusammenfassung:We investigate the coevolution of metals and dust for 173 galaxies at 4.08 presents a metal-to-stellar mass ratio larger than a few 10^-3, above a floor. This suggests a very fast rise of metals at high redshift, impacting the tentative detections of population III objects.
DOI:10.48550/arxiv.2410.23959