Low gas-phase metallicities of ultraluminous infrared galaxies are a result of dust obscurationDOI: info:10.1038/s41550-022-01679-yv. 6844–849
Chartab, Nima, Cooray, Asantha, Ma, Jingzhe, Nayyeri, Hooshang, Zilliot, Preston, Lopez, Jonathan, Fadda, Dario, Herrera-Camus, Rodrigo, Malkan, Matthew, Rigopoulou, Dimitra, Sheth, Kartik, and Wardlow, Julie. 2022. "Low gas-phase metallicities of ultraluminous infrared galaxies are a result of dust obscuration." Nature Astronomy, 6 844–849. https://doi.org/10.1038/s41550-022-01679-y.