XRISM's Resolve instrument resolves the ultra-fast outflow of quasar PDS 456 into five discrete velocity components, implying a clumpy wind with a mass outflow rate of 60-170 solar masses per year and kinetic power above 1e47 erg/s.
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Structured ionized winds shooting out from a quasar at relativistic speeds
XRISM's Resolve instrument resolves the ultra-fast outflow of quasar PDS 456 into five discrete velocity components, implying a clumpy wind with a mass outflow rate of 60-170 solar masses per year and kinetic power above 1e47 erg/s.