The high energy X-ray probe (HEX-P): Resolving the nature of Sgr A* flares, compact object binaries and diffuse X-ray emission in the Galactic center and beyond

Kaya Mori; G. Ponti; Matteo Bachetti; A. Bodaghee; J. E. Grindlay; J. Hong; R. Krivonos; Е. А. Кузнецова; Shifra Mandel; Antonio C. Rodriguez; Giovanni Stel; Shuo Zhang; Tong Bao; F. E. Bauer; M. Clavel; Benjamin M. Coughenour; Javier A. García; J. Gerber; Brian W. Grefenstette; Amruta Jaodand; B. D. Lehmer; Kristin K. Madsen; Melania Nynka; P. Predehl; Ciro Salcedo; Daniel Stern; John A. Tomsick

doi:10.3389/fspas.2023.1292130

lt;10"$ FWHM) and broad spectral coverage (0.2-80 keV) with an effective area far superior to current facilities' (including XMM-Newton and NuSTAR). These capabilities will enable revolutionary new insigh…" /> The high energy X-ray probe (HEX-P): Resolving the nature of Sgr A* flares, compact object binaries and diffuse X-ray emission in the Galactic center and beyond