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
Published in Frontiers in Astronomy and Space Sciences, 2024
Recommended citation: Kaya {Mori}, Gabriele {Ponti}, Matteo {Bachetti}, Arash {Bodaghee}, Jonathan {Grindlay}, Jaesub {Hong}, Roman {Krivonos}, Ekaterina {Kuznetsova}, Shifra {Mandel}, Antonio {Rodriguez}, Giovanni {Stel}, Shuo {Zhang}, Tong {Bao}, Franz {Bauer}, Maca {Clavel}, Benjamin {Coughenour}, Javier {Garca}, Julian {Gerber}, Brian {Grefenstette}, Amruta {Jaodand}, Bret {Lehmer}, Kristin {Madsen}, Melania {Nynka}, Peter {Predehl}, Ciro {Salcedo}, Daniel {Stern}, John {Tomsick}, "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." Frontiers in Astronomy and Space Sciences, 2024.
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