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.

Autor: Mori, Kaya1 kaya@astro.columbia.edu, Ponti, Gabriele2,3, Bachetti, Matteo4, Bodaghee, Arash5, Grindlay, Jonathan6, Jaesub Hong6, Krivonos, Roman7, Kuznetsova, Ekaterina7, Mandel, Shifra1, Rodriguez, Antonio8, Stel, Giovanni2, Shuo Zhang9, Tong Bao10, Bauer, Franz11, Clavel, Maïca12, Coughenour, Benjamin13, García, Javier A.14, Gerber, Julian1, Grefenstette, Brian8, Jaodand, Amruta8
Zdroj: Frontiers in Astronomy & Space Sciences. 2024, p01-24. 24p.
Databáze: Academic Search Ultimate
Externí odkaz:
Nepřihlášeným uživatelům se plný text nezobrazuje