The Astrophysical Journal (Jan 2025)

Multicomponent Ionized Gas Outflows in the Hot Dust-obscured Galaxy W2026+0716 with Keck/OSIRIS

  • Chao Liu,
  • Chao-Wei Tsai,
  • Peter R. M. Eisenhardt,
  • Hyunsung D. Jun,
  • Guodong Li,
  • Jingwen Wu,
  • Roberto J. Assef,
  • Andrew W. Blain,
  • Maren Cosens,
  • Tanio Díaz-Santos,
  • Román Fernández Aranda,
  • Lei Hao,
  • Mai Liao,
  • Shuai Liu,
  • Daniel Stern,
  • Andrey Vayner,
  • Shelley Wright,
  • Sherry Yeh

DOI
https://doi.org/10.3847/1538-4357/adc9b5
Journal volume & issue
Vol. 986, no. 1
p. 26

Abstract

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We present narrowband-filtered integral field unit observations of the hot dust-obscured galaxy (Hot DOG) WISE J202615.27+071624.0 (hereafter W2026+0716) at redshift z = 2.570 using Keck/OSIRIS. Our analysis reveals a multicomponent ionized gas outflow structure in this heavily obscured active galactic nucleus (AGN) host galaxy. Multicomponent Gaussian decomposition of the [O iii ] and H α emission lines uncovers extremely broad and asymmetric profiles, characteristic of AGN-driven outflows. Kinematic mapping shows spatially distinct structures: the [O iii ]- and H α -dominated components (with radii of 1.20 ± 0.56 kpc) are separated by a projected offset of ∼1.1 kpc and exhibit divergent velocity regimes. The [O iii ] outflow reaches a velocity of 3210 ± 50 km s ^−1 , while the H α outflow component attains 2310±840 km s ^−1 . Dynamical modeling supports a biconical outflow structure, with [O iii ] and H α emissions dominating separate cones and significant dust obscuration of the redshifted outflow. Their comparable momentum outflow rates and energy outflow rates suggest a potential physical connection in their driving mechanisms. Spectral energy distribution analysis reveals anomalous optical/UV excess, attributed to AGN photon scattering by dust or outflowing material, classifying W2026+0716 as a “Blue Hot DOG”. The derived outflow timescale (∼10 ^5 yr) aligns with the evolutionary phase of Blue Hot DOGs, suggesting AGN feedback operates persistently during this transitional stage.

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