2010/01/01 by T. Belloni, Tomaso M. Belloni, A. Comastri +2 · 2 citations
Engineering · Physics and Astronomy · #Accretion (finance) #Accretion disc #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Black hole (networking) #Computer science #Computer security #Connection (principal bundle) #Engineering #Gamma-ray bursts and supernovae #Physics #Pulsars and Gravitational Waves Research #astro-ph.HE
paper · pdf · doi:10.1063/1.3475157
published in AIP conference proceedings, 107-110 (American Institute of Physics) · 4 pages, 2 figures.To appear in Proceedings of "X-ray Astronomy 2009: Present Status, Multi-Wavelength Approach and Future Perspectives", Bologna, Italy, September 7-11, 2009, AIP, eds. A. Comastri, M. Cappi, and L. Angelini
openalex publication_date 2010/01/01 · arxiv created 2010/01/05 · arxiv updated 2015/05/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
I briefly outline the state‐paradigm that has emerged from the study of black‐hole binaries with RossiXTE. This is the starting point of a number of studies that address the connection between accretion and jet ejection and the physical nature of the hard spectral components in these systems.