Correcting C iv-based virial black hole masses

The C IV...1498,1501 broad emission line is visible in optical spectra to redshifts exceeding z ~ 5. C IV has long been known to exhibit significant displacements to the blue and these 'blueshifts' almost certainly signal the presence of strong outflows. As a consequence, single-epoch viri...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society 2017-02, Vol.465 (2), p.2120-2120
Hauptverfasser: Coatman, Liam, Hewett, Paul C, Banerji, Manda, Richards, Gordon T, Hennawi, Joseph F, Prochaska, J Xavier
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Sprache:eng
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