The Galactic Bulge Diffuse Emission in Broadband X-Rays with NuSTAR

The diffuse hard X-ray emission that fills the Galactic center, bulge, and ridge is believed to arise from unresolved populations of X-ray binary systems. However, the identity of the dominant class of accreting objects in each region remains unclear. Recent studies of Fe line properties and the low...

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Bibliographic Details
Main Authors: Perez, Kerstin M., Krivonos, Roman, Wik, Daniel R
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:English
Published: American Astronomical Society 2020
Online Access:https://hdl.handle.net/1721.1/128869