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Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT

  • Authors: Satoshi Yamada, Yoshihiro Ueda, Atsushi Tanimoto, Masatoshi Imanishi, Yoshiki Toba, Claudio Ricci, and George C. Privon

2021 The Astrophysical Journal Supplement Series 257 61.

  • Provider: AAS Journals

Caption: Figure 10.

Line-of-sight hydrogen column density vs. IR-based Eddington ratio. The black solid line shows the effective Eddington limit (﹩{\lambda }_{\mathrm{Edd}}^{\mathrm{eff}};﹩ Fabian et al. 2008, 2009). The pink shaded area represents the “forbidden” region obtained by the effective Eddington limit and the ﹩{N}_{{\rm{H}}}^{\mathrm{LoS}}﹩ = 1022 cm−2 limit, below which absorption by outer dust lanes may become important. Symbols and colors are the same as in Figure 3. The black open circles, open squares, and filled points mark the detections of strong molecular outflows with velocities of Vout,mol ≥ 500 km s−1 (e.g., González-Alfonso et al. 2017; Laha et al. 2018, and references therein), ionized outflows (e.g., Rich et al. 2015; Kakkad et al. 2018; Fluetsch et al. 2021), and UFOs (Mizumoto et al. 2019; Smith et al. 2019), respectively.

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