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Dave Russell (New York University Abu Dhabi)09/09/2026, 16:30Talk
X-ray binaries radiate brightly from radio to X-ray due to the accretion and ejection of matter in the system. Complex, correlated flux variations probe links between emitting components, on short as well as long timescales. Here I review the progression of multi-wavelength studies of X-ray binaries, focusing on long-term (day+ timescales) correlated behaviour between radio, optical/infrared...
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Justine Crook-Mansour (University of OXford)09/09/2026, 17:00
During the hard and quiescent spectral states in X-ray binaries, a non-linear correlation is observed between radio and X-ray luminosities, providing a valuable tool to probe the connection between accretion and jet production. This relation was originally thought to define a single ‘standard’ correlation spanning several orders of magnitude in X-ray luminosity, and was extended to active...
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