Unobscured type 2 active galactic nuclei

Yong Shi, George H. Rieke, Paul Smith, Jane Rigby, Dean Hines, Jennifer Donley, Gary Schmidt, Aleksandar M. Diamond-Stanic

Research output: Contribution to journalArticle

44 Citations (Scopus)

Abstract

Type 2 active galactic nuclei (AGNs) with intrinsically weak broad emission lines (BELs) would be exceptions to the unified model. After examining a number of proposed candidates critically, we find that the sample is contaminated significantly by objects with BELs of strengths indicating that they actually contain intermediate-type AGNs, plus a few Compton-thick sources as revealed by extremely low ratios of X-ray to nuclear IR luminosities. We develop quantitative metrics that show two (NGC3147 and NGC4594) of the remaining candidates to have BELs 2-3 orders of magnitude weaker than those of typical type1 AGNs. Several more galaxies remain as candidates to have anomalously weak BELs, but this status cannot be confirmed with the existing information. Although the parent sample is poorly defined, the two confirmed objects are well under 1% of its total number of members, showing that the absence of a BEL is possible, but very uncommon in AGN. We evaluate these two objects in detail using multi-wavelength measurements including new IR data obtained with Spitzer and ground-based optical spectropolarimeteric observations. They have little X-ray extinction with N H < ∼ 1021cm-2. Their IR spectra show strong silicate emission (NGC4594) or weak aromatic features on a generally power-law continuum with a suggestion of silicates in emission (NGC3147). No polarized BEL is detected in NGC3147. These results indicate that the two unobscured type2 objects have circumnuclear tori that are approximately face-on. Combined with their X-ray and optical/UV properties, this behavior implies that we have an unobscured view of the nuclei and thus that they have intrinsically weak BELs. We compare their properties with those of the other less-extreme candidates. We then compare the distributions of bolometric luminosities and accretion rates of these objects with theoretical models that predict weak BELs.

Original languageEnglish (US)
Pages (from-to)115-129
Number of pages15
JournalAstrophysical Journal
Volume714
Issue number1
DOIs
StatePublished - 2010

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active galactic nuclei
silicates
silicate
luminosity
x rays
optical property
suggestion
power law
extinction
accretion
galaxies
continuums
wavelength
nuclei

Keywords

  • Galaxies: nuclei
  • Galaxies: Seyfert

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Shi, Y., Rieke, G. H., Smith, P., Rigby, J., Hines, D., Donley, J., ... Diamond-Stanic, A. M. (2010). Unobscured type 2 active galactic nuclei. Astrophysical Journal, 714(1), 115-129. https://doi.org/10.1088/0004-637X/714/1/115

Unobscured type 2 active galactic nuclei. / Shi, Yong; Rieke, George H.; Smith, Paul; Rigby, Jane; Hines, Dean; Donley, Jennifer; Schmidt, Gary; Diamond-Stanic, Aleksandar M.

In: Astrophysical Journal, Vol. 714, No. 1, 2010, p. 115-129.

Research output: Contribution to journalArticle

Shi, Y, Rieke, GH, Smith, P, Rigby, J, Hines, D, Donley, J, Schmidt, G & Diamond-Stanic, AM 2010, 'Unobscured type 2 active galactic nuclei', Astrophysical Journal, vol. 714, no. 1, pp. 115-129. https://doi.org/10.1088/0004-637X/714/1/115
Shi, Yong ; Rieke, George H. ; Smith, Paul ; Rigby, Jane ; Hines, Dean ; Donley, Jennifer ; Schmidt, Gary ; Diamond-Stanic, Aleksandar M. / Unobscured type 2 active galactic nuclei. In: Astrophysical Journal. 2010 ; Vol. 714, No. 1. pp. 115-129.
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AB - Type 2 active galactic nuclei (AGNs) with intrinsically weak broad emission lines (BELs) would be exceptions to the unified model. After examining a number of proposed candidates critically, we find that the sample is contaminated significantly by objects with BELs of strengths indicating that they actually contain intermediate-type AGNs, plus a few Compton-thick sources as revealed by extremely low ratios of X-ray to nuclear IR luminosities. We develop quantitative metrics that show two (NGC3147 and NGC4594) of the remaining candidates to have BELs 2-3 orders of magnitude weaker than those of typical type1 AGNs. Several more galaxies remain as candidates to have anomalously weak BELs, but this status cannot be confirmed with the existing information. Although the parent sample is poorly defined, the two confirmed objects are well under 1% of its total number of members, showing that the absence of a BEL is possible, but very uncommon in AGN. We evaluate these two objects in detail using multi-wavelength measurements including new IR data obtained with Spitzer and ground-based optical spectropolarimeteric observations. They have little X-ray extinction with N H < ∼ 1021cm-2. Their IR spectra show strong silicate emission (NGC4594) or weak aromatic features on a generally power-law continuum with a suggestion of silicates in emission (NGC3147). No polarized BEL is detected in NGC3147. These results indicate that the two unobscured type2 objects have circumnuclear tori that are approximately face-on. Combined with their X-ray and optical/UV properties, this behavior implies that we have an unobscured view of the nuclei and thus that they have intrinsically weak BELs. We compare their properties with those of the other less-extreme candidates. We then compare the distributions of bolometric luminosities and accretion rates of these objects with theoretical models that predict weak BELs.

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