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19972019
most citedThe Mass-Metallicity relation explored with CALIFA: I. Is there a dependence on the star formation rate?

276 citations · 1.9k across the 31 of their papers we have counts for

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10 papers · 1 filter

astro-ph2008

Fueling QSOs: The Relevance of Mergers

Nicola Bennert, Gabriela Canalizo, Bruno Jungwiert +4

To study the relevance of mergers for the fueling of QSOs, we are currently conducting an HST imaging campaign of a sample of QSO host galaxies classified as ellipticals in the lit…

astro-ph2008★ 158 cited

Evidence for Merger Remnants in Early-Type Host Galaxies of Low-Redshift QSOs

Nicola Bennert, Gabriela Canalizo, Bruno Jungwiert +4

We present results from a pilot HST ACS deep imaging study in broad-band V of five low-redshift QSO host galaxies classified in the literature as ellipticals. The aim of our study…

astro-ph2007

Searching for Mergers in Early-Type QSO Host Galaxies and a Control Sample of Inactive Ellipticals

Nicola Bennert, Gabriela Canalizo, Bruno Jungwiert +4

We present very deep HST/ACS images of five QSO host galaxies, classified as undisturbed ellipticals in earlier studies. For four of the five objects, our images reveal strong sign…

astro-ph2007★ 79 cited

Spectacular Shells in the Host Galaxy of the QSO MC2 1635+119

Gabriela Canalizo, Nicola Bennert, Bruno Jungwiert +4

We present deep HST/ACS images and Keck spectroscopy of MC2 1635+119, a QSO hosted by a galaxy previously classified as an undisturbed elliptical. Our new images reveal dramatic sh…

astro-ph2006

Properties of the Narrow-Line Region in Seyfert Galaxies

Nicola Bennert, Bruno Jungwiert, Stefanie Komossa +3

We study the narrow-line region (NLR) of six Seyfert-1 and six Seyfert-2 galaxies by means of spatially resolved optical spectroscopy and photoionization modelling. From spatially…

astro-ph2006★ 144 cited

Size and properties of the narrow-line region in Seyfert-1 galaxies from spatially-resolved optical spectroscopy

Nicola Bennert, Bruno Jungwiert, Stefanie Komossa +3

Spatially resolved emission-line spectroscopy is a powerful tool to determine the physical conditions in the narrow-line region (NLR) of active galactic nuclei (AGNs). We recently…