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A strong He II $λ$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Wang, Xin, Cheng, Cheng, Ge, Junqiang, Meng, Xiao-Lei, Daddi, Emanuele, Yan, Haojing, Ji, Zhiyuan, Jin, Yifei, Jones, Tucker, Malkan, Matthew A., Haro, Pablo Arrabal, Brammer, Gabriel, Oguri, Masamune, Hou, Meicun, Zhang, Shiwu
Format:	Preprint
Publié:	2022
Sujets:	Astrophysics of Galaxies
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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