An XMM-Newton Analysis of the Supermassive Black Hole Binary Candidate MCG+11–11–032
We investigate the possibility of a binary supermassive black hole system at the center of MCG+11–11–032, a local ( z = 0.036) Seyfert 2 galaxy. Prior work with stacked Swift/XRT spectra suggested the presence of two Fe K α lines (at 6.16 and 6.56 keV) with 2 σ confidence. This could be consistent w...
Guardat en:
| Autors principals: | , , , , |
|---|---|
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
IOP Publishing
2026-01-01
|
| Col·lecció: | The Astrophysical Journal |
| Matèries: | |
| Accés en línia: | https://doi.org/10.3847/1538-4357/ae5d35 |
| Etiquetes: |
Sense etiquetes, Sigues el primer a etiquetar aquest registre!
|