论文信息 - The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources - 字舞流文

The High Energy X-ray Probe (HEX-P): Studying Extreme Accretion with Ultraluminous X-ray Sources

Center for Computational Sciences | S. O. Physics | C. I. O. Technology. | J. P. Laboratory | Cnrs | U. Hertfordshire | U. Tsukuba | M. Bachetti | G. Vasilopoulos | B. Lehmer | F. Pintore | I. Roma | M. Pilia | K. Mori | NASA's Goddard Space Flight Center | U. Toulouse | C. Maitra | Columbia Astrophysics Laboratory | Kapodistrian University of Athens | M. Brightman | U. O. H. Kong | I. Brera | K. Ohsuga | Irap | C. F. A. Physics | C. University | A. G'urpide | Cnes | H. Earnshaw | Max-Planck-Institut fur extraterrestrische Physik | X-ray Astrophysics Laboratory | Centre of Astrophysics Research | U. Arkansas | R. Amato | University of Palermo | A. Jaodand | E. Ambrosi | S. Mandel | Cahill Center for Astrophysics | Department of Physics | D. Walton | Astronomy | National | K. Madsen | D. Stern | Ciro Pinto | M. Middleton | T. P. Roberts | J. Alford | Lixin Dai | Hamza El Byad Javier A. Garc'ia | Gian Luca Israel | G. Younes | Anna Wolter INAF-Osservatorio Astronomico di Cagliari | D. University