Orbital modulations of H-like Fe, Ca, Ar, and S Ly-alpha lines in Cyg X-3 show Fe ions concentrated near the compact object and S ions more extended, yielding a stellar-wind mass-loss rate of 5e-6 to 1e-5 solar masses per year from comparison to a UV-driven wind model.
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The line modulations of H-like Fe, Ca, Ar, and S observed with $XRISM$/Resolve in Cyg X-3
Orbital modulations of H-like Fe, Ca, Ar, and S Ly-alpha lines in Cyg X-3 show Fe ions concentrated near the compact object and S ions more extended, yielding a stellar-wind mass-loss rate of 5e-6 to 1e-5 solar masses per year from comparison to a UV-driven wind model.