The Dependence of Iron-rich Metal-poor Star Occurrence on Galactic Environment Supports an Origin in Thermonuclear Supernova Nucleosynthesis

It has been suggested that a class of chemically peculiar metal-poor stars called iron-rich metal-poor (IRMP) stars formed from molecular cores with metal contents dominated by thermonuclear supernova nucleosynthesis. If this interpretation is accurate, then IRMP stars should be more common in envir...

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Bibliografische gegevens

Hoofdauteurs:	Zachary Reeves, Kevin C. Schlaufman, Henrique Reggiani
Formaat:	Artigo
Taal:	Inglês
Gepubliceerd in:	IOP Publishing 2023-01-01
Reeks:	The Astronomical Journal
Onderwerpen:	Chemical enrichment Chemically peculiar stars Dwarf spheroidal galaxies Galactic archaeology Globular star clusters Large Magellanic Cloud
Online toegang:	https://doi.org/10.3847/1538-3881/ace68d
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