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Using GALEX UV Excess to Search for Metal-poor Halo Stars

Metal-poor solar-type stars display a significant reduction in metal-line blanketing at short wavelengths, leading to an excess of near-ultraviolet (NUV) flux compared to their metal-rich counterparts. We utilize Galaxy Evolution Explorer Satellite (GALEX) NUV and Gaia DR3 photometry along with grou...

Deskribapen osoa

Gorde:
Egile Nagusiak: Chase L. Smith, Maxwell Moe, Megan Frank, Raven Cilley, Javier Fregoso, Alexander Gleason, Ella Morton, Grace Nelson, Mary Kate Petrykovets, Daniel Reshan, Kaitlyn Schultz, Daniel A. Dale, Nikhil Patten
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2026-01-01
Saila:The Astrophysical Journal
Gaiak:
Stellar abundances
Dwarf stars
Population II stars
Halo stars
Milky Way stellar halo
Ultraviolet astronomy
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ae74c3
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