Session

Multi-wavelength, Jets & Winds. Session 3.3: MW Correlation

9 Sept 2026, 16:30
Cefalù

Cefalù

Cefalù, province of Palermo, Sicily. Sala delle Capriate in the Town Hall (Piazza Duomo).

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  1. Dave Russell (New York University Abu Dhabi)
    09/09/2026, 16:30
    Talk

    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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  2. 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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