Blueshifted C IV emission in quasars requires wind mass-loading ϵ_w/f_V ∼ 50, disfavouring smooth disc winds in favour of clumpy or ambient-swept outflows.
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How massive and clumpy must a quasar wind be to create emission line blueshifts?
Blueshifted C IV emission in quasars requires wind mass-loading ϵ_w/f_V ∼ 50, disfavouring smooth disc winds in favour of clumpy or ambient-swept outflows.