True Pair-instability Supernova Descendant: Implications for the First Stars’ Mass Distribution

The initial mass function (IMF) of the first Population III (Pop III) stars remains a persistent mystery. Their predicted massive nature implies the existence of stars exploding as pair-instability supernovae (PISNe), but no observational evidence had been found. Now, the LAMOST survey claims to hav...

Deskribapen osoa

Xehetasun bibliografikoak

Egile Nagusiak:	Ioanna Koutsouridou, Stefania Salvadori, Ása Skúladóttir
Formatua:	Artigo
Hizkuntza:	Inglês
Argitaratua:	IOP Publishing 2024-01-01
Saila:	The Astrophysical Journal Letters
Gaiak:	Population III stars Milky Way evolution Galaxy evolution Galaxy formation Milky Way formation Theoretical models
Sarrera elektronikoa:	https://doi.org/10.3847/2041-8213/ad2466
Etiketak:	Etiketa erantsi Etiketarik gabe, Izan zaitez lehena erregistro honi etiketa jartzen!