2012
DOI: 10.1007/s10511-012-9252-7
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Dust obscuration of the narrow line region of active galactic nuclei

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Cited by 4 publications
(3 citation statements)
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“…We note that Sargsyan et al (2012) have noticed large [CII]/PAH ratios, particularly in galaxies with known AGN. In this case, extinction in the mid-IR was cited as a possible explanation, although no deep silicate features were observed.…”
Section: X-ray Heating?mentioning
confidence: 68%
“…We note that Sargsyan et al (2012) have noticed large [CII]/PAH ratios, particularly in galaxies with known AGN. In this case, extinction in the mid-IR was cited as a possible explanation, although no deep silicate features were observed.…”
Section: X-ray Heating?mentioning
confidence: 68%
“…1. AGN lack detectable NLRs because of obscuration by dust in the host galaxy (Rigby et al 2006;Goulding & Alexander 2009;Trump et al 2009;Sargsyan et al 2012).…”
Section: Bpt-hii As Agn With Intrinsically No Emission Lines or With ...mentioning
confidence: 99%
“…The importance of this conclusion lies in the possibility of interpreting these off-equatorial tori as forming the surrounding material usually invoked to explain the spectral emission/absorption features in accretiondisc systems. Possible examples of this type are provided by coronal halos consisting of non-neutral ion-electron plasmas or by obscuring dusty-plasma tori that are believed to be produced in galactic nuclei (Sargsyan et al 2012;Goulding et al 2012;Dorodnitsyn et al 2011;Mor et al 2011;Kawaguchi et al 2011;Oyabu et al 2011;Hatziminaoglou et al 2009;Mor et al 2009;Fabian et al 2008;Hönig et al 2007).…”
Section: Introductionmentioning
confidence: 99%