Distinct Accretion Modes of Cygnus X-1 Revealed from Hard X-Rays
Author:
Funder
National Polish Science Centre
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab9311/pdf
Reference58 articles.
1. Thermal equilibria of accretion disks
2. X-ray variability in a deep, flux-limited sample of QSOs
3. ACCRETION DISK DYNAMO AS THE TRIGGER FOR X-RAY BINARY STATE TRANSITIONS
4. States and Transitions in Black Hole Binaries
5. Transient Black Hole Binaries
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1. What Is the Black Hole Spin in Cyg X-1?;The Astrophysical Journal Letters;2024-05-01
2. High Hard X-Ray Polarization in Cygnus X-1 Confined to the Intermediate Hard State: Evidence for a Variable Jet Component;The Astrophysical Journal Letters;2023-12-29
3. The INTEGRAL view on black hole X-ray binaries;New Astronomy Reviews;2021-12
4. Detection of a Low-frequency Quasi-periodic Oscillation in the Soft State of Cygnus X-1 with Insight-HXMT;The Astrophysical Journal;2021-09-01
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