We present a simple population synthesis scheme which recognizes composite starburst+Seyfert 2 nuclei from a few easy-to-obtain optical measurements. Composite systems seem to evolve towards less luminous Seyfert 2's which do not harbor detectable circum-nuclear starbursts. We encourage applications of this cheap diagnostic tool to large samples of Seyfert 2's, as well as its extension to other activity classes, in order to test and refine this evolutionary scenario
We investigate the relation between the characteristics of the circumnuclear stellar population and ...
We present near-infrared spectra for a sample of galaxies with ambiguous optical emission-line ratio...
We discuss BeppoSAX observations and archive ASCA data of NGC 7679, a nearby, nearly face-on SB0 gal...
We examine a representative sample of 35 Seyfert 2 nuclei. Previous work has shown that nearly half ...
Observations at ultraviolet, optical and near-infrared wavelengths have shown the existence of recen...
There is ever mounting evidence for a connection between the evolution of AGN and starburst-activity...
We report the results of a spectroscopic investigation of a sample of 20 of the brightest type 2 Sey...
This paper presents new Chandra and BeppoSAX observations aimed at investigating the optical/X-ray m...
Two main physical processes characterize the activity in the nuclear region of active galaxies: an i...
Observational diagnostics for the recognition of circumnuclear star formation in Seyfert galaxies ar...
Nuclear activity and star formation processes represent two key elements in the evolution of galaxie...
Active galactic nuclei (Seyfert nuclei and their relatives) and intense star formation can both deli...
We stress the importance of Wolf-Rayet stars for the understanding of the AGN phenomenon in galaxies...
We compare the arcsecond-scale circumnuclear radio continuum properties of five Seyfert and five sta...
We analyze the physical properties of post-starburst AGN SDSS J085338.27+033246.1 according to its o...
We investigate the relation between the characteristics of the circumnuclear stellar population and ...
We present near-infrared spectra for a sample of galaxies with ambiguous optical emission-line ratio...
We discuss BeppoSAX observations and archive ASCA data of NGC 7679, a nearby, nearly face-on SB0 gal...
We examine a representative sample of 35 Seyfert 2 nuclei. Previous work has shown that nearly half ...
Observations at ultraviolet, optical and near-infrared wavelengths have shown the existence of recen...
There is ever mounting evidence for a connection between the evolution of AGN and starburst-activity...
We report the results of a spectroscopic investigation of a sample of 20 of the brightest type 2 Sey...
This paper presents new Chandra and BeppoSAX observations aimed at investigating the optical/X-ray m...
Two main physical processes characterize the activity in the nuclear region of active galaxies: an i...
Observational diagnostics for the recognition of circumnuclear star formation in Seyfert galaxies ar...
Nuclear activity and star formation processes represent two key elements in the evolution of galaxie...
Active galactic nuclei (Seyfert nuclei and their relatives) and intense star formation can both deli...
We stress the importance of Wolf-Rayet stars for the understanding of the AGN phenomenon in galaxies...
We compare the arcsecond-scale circumnuclear radio continuum properties of five Seyfert and five sta...
We analyze the physical properties of post-starburst AGN SDSS J085338.27+033246.1 according to its o...
We investigate the relation between the characteristics of the circumnuclear stellar population and ...
We present near-infrared spectra for a sample of galaxies with ambiguous optical emission-line ratio...
We discuss BeppoSAX observations and archive ASCA data of NGC 7679, a nearby, nearly face-on SB0 gal...