An Indication of Gas Inflow in Clumpy Star-Forming Galaxies near $z\sim 1$: Lower Gas-Phase Metallicities in Clumpy Galaxies Compared to Non-Clumpy Galaxies

Visal Sok, Adam Muzzin, Pascale Jablonka +5

Despite the ubiquity of clumpy star-forming galaxies at high-redshift, the origin of clumps are still largely unconstrained due to the limited observations that can validate the me…