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The Origin of the Nuclear Star-forming Ring in NGC 3182

  • Authors: Mina Pak, Joon Hyeop Lee, Hyunjin Jeong, Woong-Seob Jeong

Mina Pak et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 6.

In the top, Hα, Hβ, [S II], [O III], and [N II] line flux (10−17 erg s−1 cm−2) and line-ratio maps of NGC 3182 are presented. In the bottom, we present emission-line-ratio diagrams and maps for [O III]5007/Hβ vs. [N II]6583/Hα and [O III]5007/Hβ vs. [S II]6731/Hα color coded by ionization source. The representative uncertainties are shown bottom right corner of each panel. Lines in the diagrams are from Kauffmann et al. (2003) and Sharp & Bland-Hawthorn (2010), respectively, to separate star forming, the AGN, and LINERs. Circles are the same as in Figure 4.

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