activity
19972018
most citedProperties of flat-spectrum radio-loud Narrow-Line Seyfert 1 Galaxies

164 citations · 1.2k across the 51 of their papers we have counts for

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8 papers · 1 filter

astro-ph.CO2013

Are Boltzmann Plots of Hydrogen Balmer lines a tool for identifying a subclass of S1 AGN?

P. Rafanelli, S. Ciroi, V. Cracco +4

It is becoming clear that we can define two different types of nearby AGN belonging to the Seyfert 1 class (S1), on the basis of the match of the intensities of their Broad Balmer…

astro-ph.CO2012★ 64 cited

Spectral properties of the narrow-line region in Seyfert galaxies selected from the SDSS-DR7

L. Vaona, S. Ciroi, F. Di Mille +3

Although the properties of the narrow-line region (NLR) of active galactic nuclei(AGN) have been deeply studied by many authors in the past three decades, many questions are still…

astro-ph.CO2012★ 3 cited

The Relation between Nuclear Activity and Stellar Mass in Galaxies

G. La Mura, D. Bindoni, S. Ciroi +4

The existence of correlations between nuclear properties of galaxies, such as the mass of their central black holes, and larger scale features, like the bulge mass and luminosity,…

astro-ph.CO2012★ 32 cited

The analysis of the hydrogen broad Balmer line ratios: possible implications to the physical properties of the BLR of AGN

D. Ilic, L. C. Popovic, G. La Mura +2

We analyze the ratios of the broad hydrogen Balmer emission lines (from Hαto Hε) in the context of estimating the physical conditions in the broad line region (BLR) of active galac…

astro-ph.CO2011★ 16 cited

The origin of gas in the Extended Narrow Line Region of nearby Seyfert galaxies.I. NGC 7212

V. Cracco, S. Ciroi, F. Di Mille +6

The Extended Narrow Line Region (ENLR) of Active Galactic Nuclei (AGN) is a region of highly ionized gas with a size of few up to 15-20 kpc. When it shows a conical or bi-conical s…

astro-ph.CO2010

The nature of gas and stars in the circumnuclear regions of AGN: a chemical approach

P. Rafanelli, L. Vaona, R. D'Abrusco +2

Aim of this communication is to describe the first results of a work-in-progress regarding the chemical properties of gas and stars in the circumnuclear regions of nearby galaxies.…