activity
20052022
most citedMolecular gas in nearby low-luminosity QSO host galaxies

81 citations · 402 across the 24 of their papers we have counts for

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Showing 2013Show all

7 papers · 1 filter

astro-ph.GA2013★ 3 cited

The Galactic Center as a Paradigm for Low Luminosity Nuclei? The K-band identification of the DSO/G2 source from VLT and Keck data

Andreas Eckart, S. Britzen, M. Horrobin +27

The super-massive 4 million solar mass black hole (SMBH) SgrA* shows flare emission from the millimeter to the X-ray domain. The nucleus of the Milky Way has properties (stellar cl…

astro-ph.CO2013★ 40 cited

A low-luminosity type-1 QSO sample: I. Overluminous host spheroidals or undermassive black holes?

Gerold Busch, Jens Zuther, Mónica Valencia-S. +6

Recognizing the properties of the host galaxies of quasi-stellar objects (QSOs) is essential to understand the suspected coevolution of central supermassive black holes (BHs) and t…

astro-ph.CO2013

A low-redshift low luminosity QSO sample: Comparison with NUGA galaxies and PG QSOs and first interferometric images of three sample members

Lydia Moser, Jens Zuther, Sebastian Fischer +5

The low luminosity QSO (LLQSO) sample consists of type 1 active galactic nuclei (AGN) up to a redshift of z=0.06 in the Hamburg/ESO QSO survey. Its purpose is to study how the brig…

astro-ph.CO2013★ 15 cited

What produces the extended LINER-type emission in the NUGA galaxy NGC 5850?

Marcus Bremer, Julia Scharwächter, Andreas Eckart +5

(Abridged) The role of low ionization nuclear emission region (LINER) galaxies within the picture of active galactic nuclei (AGN) has been controversial. It is still not clear whet…

astro-ph.CO2013

The central kpc of edge-on AGN

Semir Smajić, Sebastian Fischer, Jenz Zuther +2

The NIR is less influenced by dust extinction than optical light. This enables us to look to an extent through dusty regions. In addition, it is sensitive to the mass-dominating st…

astro-ph.CO2013★ 1 cited

Discovery of an Intermediate Mass Black Hole at the center of the starburst/Seyfert composite galaxy IRAS 01072+4954

M. Valencia-S., A. Eckart, J. Zuther +8

The starburst/Seyfert composite galaxy IRAS 01072+4954 (z=0.0236) is an enigmatic source that combines a Seyfert~1-like X-ray emission with a starburst optical spectrum that lacks…