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Elemental Abundances in X-Ray Binary Outflows

Line-resolved X-ray spectra of outflows from X-ray binaries are interesting since they provide quantifiable measures of the accreted material onto the compact object (black hole or neutron star), which can not be observed directly in the accretion disk. One such measurement that has been largely ove...

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Detalles Bibliográficos
Principais autores: Noa Keshet, Ehud Behar, Jon M. Miller
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
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Acceso en liña:https://doi.org/10.3847/1538-4357/adfa9b
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