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- W1591857335 abstract "The Spitzer high resolution spectra of 72 Seyfert galaxies from the 12$mu$m Galaxy Sample are presented and discussed. The presence of starburst components in these galaxies can be quantified by powerful mid-IR diagnostics tools (i.e. 11.25$mu$m PAH feature equivalent width and the H$_2$ emission line intensity), as well as the AGN dominance can be measured by specific fine structure line ratios (e.g. [NeV]/[NeII], [NeV]/[SiII], etc.). The two types of Seyfert galaxies do not show any statistical difference in our diagnostic tools. However, the Seyfert 2's showing hidden Broad Line Regions in spectro-polarimetric observations have on average an higher AGN dominance, a weaker star formation component and a warmer [60 - 25] spectral index than those without broad emission lines." @default.
- W1591857335 created "2016-06-24" @default.
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- W1591857335 date "2008-07-30" @default.
- W1591857335 modified "2023-09-23" @default.
- W1591857335 title "Seyfert Galaxies in the Local Universe: Analysis of Spitzer Spectra of a Complete Sample" @default.
- W1591857335 hasPublicationYear "2008" @default.
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