Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$

Fuente: arXiv
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Bibliographic Details
Main Authors: Dessauges-Zavadsky, M., Marques-Chaves, R., Schaerer, D., Xiao, M. -Y., Colina, L., Alvarez-Marquez, J., Pérez-Fournon, I.
Format: Preprint
Published: 2024
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