Resolving the Fe Kα Doublet of the Galactic Center Molecular Cloud G0.11-0.11 with XRISM

Fe K α line emission from Galactic center molecular clouds can be produced either via fluorescence after illumination by an X-ray source or by cosmic-ray ionization. Unparalleled high-resolution X-ray spectroscopy obtained by XRISM/Resolve for the Galactic center molecular cloud G0.11-0.11 resolves...

Descripció completa

Dades bibliogràfiques

Autors principals:	Stephen DiKerby, Shuo Zhang, Kumiko K. Nobukawa, Masayoshi Nobukawa, Yuma Aoki, Jack Uteg
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2026-01-01
Col·lecció:	The Astrophysical Journal Letters
Matèries:	Molecular clouds Galactic center High resolution spectroscopy X-ray astronomy
Accés en línia:	https://doi.org/10.3847/2041-8213/ae331c
Etiquetes:	Afegir etiqueta Sense etiquetes, Sigues el primer a etiquetar aquest registre!