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• W4306180848 endingPage "87" @default.
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• W4306180848 abstract "Abstract To understand the origin of nuclear (≲100 pc) millimeter-wave (mm-wave) continuum emission in active galactic nuclei (AGNs), we systematically analyzed subarcsecond resolution Band-6 (211–275 GHz) Atacama Large Millimeter/submillimeter Array data of 98 nearby AGNs ( z < 0.05) from the 70 month Swift/BAT catalog. The sample, almost unbiased for obscured systems, provides the largest number of AGNs to date with high mm-wave spatial resolution sampling (∼1–200 pc), and spans broad ranges of 14–150 keV luminosity { <?CDATA $40lt mathrm{log}[{L}_{14-150}/(mathrm{erg},{{rm{s}}}^{-1})]lt 45$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mn>40</mml:mn> <mml:mo><</mml:mo> <mml:mi>log</mml:mi> <mml:mo stretchy=false>[</mml:mo> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mn>14</mml:mn> <mml:mo>−</mml:mo> <mml:mn>150</mml:mn> </mml:mrow> </mml:msub> <mml:mrow> <mml:mo stretchy=true>/</mml:mo> </mml:mrow> <mml:mo stretchy=false>(</mml:mo> <mml:mi>erg</mml:mi> <mml:mspace width=0.25em /> <mml:msup> <mml:mrow> <mml:mi mathvariant=normal>s</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow> </mml:msup> <mml:mo stretchy=false>)</mml:mo> <mml:mo stretchy=false>]</mml:mo> <mml:mo><</mml:mo> <mml:mn>45</mml:mn> </mml:math> }, black hole mass <?CDATA $[5lt mathrm{log}({M}_{mathrm{BH}}/{M}_{odot })lt 10$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mo stretchy=false>[</mml:mo> <mml:mn>5</mml:mn> <mml:mo><</mml:mo> <mml:mi>log</mml:mi> <mml:mo stretchy=false>(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>BH</mml:mi> </mml:mrow> </mml:msub> <mml:mrow> <mml:mo stretchy=true>/</mml:mo> </mml:mrow> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo stretchy=false>)</mml:mo> <mml:mo><</mml:mo> <mml:mn>10</mml:mn> </mml:math> ], and Eddington ratio ( <?CDATA $-4lt mathrm{log}{lambda }_{mathrm{Edd}}lt 2$?> <mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML overflow=scroll> <mml:mo>−</mml:mo> <mml:mn>4</mml:mn> <mml:mo><</mml:mo> <mml:mi>log</mml:mi> <mml:msub> <mml:mrow> <mml:mi>λ</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>Edd</mml:mi> </mml:mrow> </mml:msub> <mml:mo><</mml:mo> <mml:mn>2</mml:mn> </mml:math> ). We find a significant correlation between 1.3 mm (230 GHz) and 14–150 keV luminosities. Its scatter is ≈0.36 dex, and the mm-wave emission may serve as a good proxy of the AGN luminosity, free of dust extinction up to N H ∼ 10 26 cm −2 . While the mm-wave emission could be self-absorbed synchrotron radiation around the X-ray corona according to past works, we also discuss different possible origins of the mm-wave emission: AGN-related dust emission, outflow-driven shocks, and a small-scale (<200 pc) jet. The dust emission is unlikely to be dominant, as the mm-wave slope is generally flatter than expected. Also, due to no increase in the mm-wave luminosity with the Eddington ratio, a radiation-driven outflow model is possibly not the common mechanism. Furthermore, we find independence of the mm-wave luminosity on indicators of the inclination angle from the polar axis of the nuclear structure, which is inconsistent with a jet model whose luminosity depends only on the angle." @default.
• W4306180848 created "2022-10-14" @default.
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• W4306180848 date "2022-10-01" @default.
• W4306180848 modified "2023-10-10" @default.
• W4306180848 title "BASS XXXII: Studying the Nuclear Millimeter-wave Continuum Emission of AGNs with ALMA at Scales ≲100–200 pc" @default.
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