An Indication of Gas Inflow in Clumpy Star-Forming Galaxies near $z\sim1$: Lower Gas-Phase Metallicities in Clumpy Galaxies Compared to Non-Clumpy Galaxies

Fuente: arXiv

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Bibliographic Details
Main Authors:	Sok, Visal, Muzzin, Adam, Jablonka, Pascale, Tan, Vivian Yun Yan, Marsan, Z. Cemile, Marchesini, Danilo, Wilson, Gillian, Alcorn, Leo Y.
Format:	Preprint
Published:	2024
Subjects:	Astrophysics of Galaxies
Online Access:	Acceder al recurso
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