作者: David S. N. Rupke , Kayhan Gültekin , Sylvain Veilleux
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摘要: The prevalence and properties of kiloparsec-scale outflows in nearby Type 1 quasars have been the subject little previous attention. This work presents Gemini integral field spectroscopy ten radio-quiet at $z $1000 M$_\odot$/yr) momentum boosts [($c$ $dp/dt$)/L$_\mathrm{AGN}$ = 0.01-20]. After extending mass scale to Seyferts, $dM/dt$ $dE/dt$ correlate with black hole ($dM/dt \sim M_\mathrm{BH}^{0.7\pm0.3}$ $dE/dt M_\mathrm{BH}^{1.3\pm0.5}$). Thus, most massive holes local universe power energetic quasar-mode winds.