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...
Main Authors: | , , |
---|---|
Other Authors: | |
Format: | Article |
Language: | English |
Published: |
American Astronomical Society,
2020-12-21T15:24:26Z.
|
Subjects: | |
Online Access: | Get fulltext |