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Autor:
T Gessey-Jones, N S Sartorio, A Fialkov, G M Mirouh, M Magg, R G Izzard, E de Lera Acedo, W J Handley, R Barkana
Properties of the first generation of stars [referred to as the Population III (Pop III) stars], such as their initial mass function (IMF), are poorly constrained by observations and have yet to converge between simulations. The cosmological 21-cm si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28bfaf4f173aeb70a4ccad23d39939ab
http://arxiv.org/abs/2202.02099
http://arxiv.org/abs/2202.02099
