GAS KINEMATICS AND PHOTOIONIZATION IN TYPE 1 AGNs WITH STRONG OUTFLOWS

  • KIM, CHANGSEOK (Astronomy Program, Department of physics and Astronomy, Seoul National University) ;
  • WOO, JONG-HAK (Astronomy Program, Department of physics and Astronomy, Seoul National University) ;
  • LUO, RONGXIN (Shanghai Astronomical Observatory)
  • Published : 2020.10.13

Abstract

We present spatially resolved outflows and photoionization for a pilot sample of 11 type 1 AGNs (z<0.3) based on the Gemini Multi-Object Spectrograph Integral Field Unit data. These AGNs were selected since we found strong outflow signatures in SDSS spectra. We focus on [OIII] and Hα emission lines to probe outflow kinematics by measuring line flux, velocity, and velocity dispersion at each pixel. We investigate characteristics of gas kinematics of type 1 AGNs and compare them with those of type 2 AGNs in our previous studies. Furthermore, by drawing BPT map, photoionization states will be also discussed. Based on the results, we discuss various implications on the impacts of outflows on star formation in host galaxies.

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