Deconstructing the Quiescent Black Hole V404 Cyg
The black hole binary V404 Cyg has provided a primary test bed for models of accretion in quiescent black hole binaries because it is by far the brightest in the X-ray band. Most published work, however, has been based on non-simultaneous data spanning many years since its major outburst in 1989. We present the most complete spectral energy
Hynes, Robert I. et al.
Advertised on:
9
2006