SIMBAD references

2006MNRAS.366..480G - Mon. Not. R. Astron. Soc., 366, 480-490 (2006/February-3)

Emission-line properties of Seyfert 2 nuclei.

GU Q., MELNICK J., CID FERNANDES R., KUNTH D., TERLEVICH E. and TERLEVICH R.

Abstract (from CDS):

This is the third paper of a series devoted to the study of the global properties of Joguet's sample of 79 nearby galaxies observable from the southern hemisphere, of which 65 are Seyfert 2 galaxies. We use the population synthesis models of Paper II to derive `pure' emission-line spectra for the Seyfert 2 galaxies in the sample, and thus explore the statistical properties of the nuclear nebular components and their relation to the stellar populations. We find that the emission-line clouds suffer substantially more extinction than the starlight, and we confirm the correlations between stellar and nebular velocity dispersions and between emission-line luminosity and velocity dispersions, although with substantial scatter. Nuclear luminosities correlate with stellar velocity dispersions, but Seyferts with conspicuous star-forming activity deviate systematically towards higher luminosities. Removing the contribution of young stars to the optical continuum produces a tighter and steeper relation, L∝σ4*, consistent with the Faber-Jackson law.

Emission-line ratios indicative of the gas excitation such as [Oiii]/Hβ and [Oiii]/[Oii] are statistically smaller for Seyferts with significant star formation, implying that ionization by massive stars is responsible for a substantial and sometimes even a dominant fraction of the Hβ and [Oii] fluxes. We use our models to constrain the maximum fraction of the ionizing power that can be generated by a hidden active galactic nucleus (AGN). We correlate this fraction with classical indicators of AGN photoionization (i.e. X-ray luminosity and nebular excitation), but find no significant correlations. Thus, while there is a strong contribution of starbursts to the excitation of the nuclear nebular emission in low-luminosity Seyferts, the contribution of the hidden AGN remains elusive even in hard X-rays.


Abstract Copyright: 2005 The Authors. Journal compilation © 2005 RAS

Journal keyword(s): galaxies: active - galaxies: Seyfert - galaxies: starburst - galaxies: statistics

VizieR on-line data: <Available at CDS (J/MNRAS/366/480): table1.dat>

Status at CDS:  

Simbad objects: 68

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2020.06.01-05:09:56

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