Evidence of Pop III stars’ chemical signature in neutral gas at z [approximately] 6 - a study based on the E-XQR-30 spectroscopic sample - Sodini, Alessio; D’Odorico, Valentina; Salvadori, Stefania; Vanni, Irene; Bischetti, Manuela; Cupani, Guido; Davies, Rebecca; Becker, George D.; Bañados, Eduardo; Bosman, Sarah; Davies, Frederick; Farina, Emanuele Paolo; et al. (Astronomy and astrophysics, 2024)
Online veröffentlicht: 31. Juli 2024