Add to ORKGWe present preliminary results from the first interferometric observations of the distribution of molecular gas in the central few kiloparsecs of Mrk 590, which in recent years has surprisingly transitioned from a Seyfert 1 to a Seyfert 1.9 or 2 galaxy
Using new Atacama Pathfinder Experiment and James Clerk Maxwell Telescope spectroscopy of the CO 2→1...
ALMA observations have revealed nuclear dusty molecular disks or tori with characteristic sizes 15-4...
In order to investigate circumnuclear molecular gaseous contents and their relation to the nuclear a...
Optical changing-look Active Galactic Nuclei (AGN) are a class of sources that change type within a ...
Active galactic nucleus (AGN) driven outflows are believed to play an important role in regulating t...
grantor: University of TorontoIn this work we examine the physical conditions of the globa...
We present near-infrared and optical emission-line and stellar kinematics of the Seyfert 2 galaxy Mr...
We use high-resolution (0.5 arcsec) CO(2-1) observations performed with the Atacama Large Millimetre...
Context. The host galaxy conditions for rapid supermassive black hole growth are poorly understood. ...
We present an investigation of possible fueling mechanisms operating in the inner kiloparsec of Seyf...
In this report we present the results of a single dish study of the molecular gas properties in Seyf...
Post-starbursts (PSBs) are candidate for rapidly transitioning from starbursting to quiescent galaxi...
Near-infrared and optical spectroscopy of the nuclear and extended emission region of the Seyfert2 g...
International audienceContext. The study of the distribution, morphology, and kinematics of cold mol...
We report ALMA observations of CO(3–2) emission in the Seyfert 2 galaxy NGC 1433 at the un...
Using new Atacama Pathfinder Experiment and James Clerk Maxwell Telescope spectroscopy of the CO 2→1...
ALMA observations have revealed nuclear dusty molecular disks or tori with characteristic sizes 15-4...
In order to investigate circumnuclear molecular gaseous contents and their relation to the nuclear a...
Optical changing-look Active Galactic Nuclei (AGN) are a class of sources that change type within a ...
Active galactic nucleus (AGN) driven outflows are believed to play an important role in regulating t...
grantor: University of TorontoIn this work we examine the physical conditions of the globa...
We present near-infrared and optical emission-line and stellar kinematics of the Seyfert 2 galaxy Mr...
We use high-resolution (0.5 arcsec) CO(2-1) observations performed with the Atacama Large Millimetre...
Context. The host galaxy conditions for rapid supermassive black hole growth are poorly understood. ...
We present an investigation of possible fueling mechanisms operating in the inner kiloparsec of Seyf...
In this report we present the results of a single dish study of the molecular gas properties in Seyf...
Post-starbursts (PSBs) are candidate for rapidly transitioning from starbursting to quiescent galaxi...
Near-infrared and optical spectroscopy of the nuclear and extended emission region of the Seyfert2 g...
International audienceContext. The study of the distribution, morphology, and kinematics of cold mol...
We report ALMA observations of CO(3–2) emission in the Seyfert 2 galaxy NGC 1433 at the un...
Using new Atacama Pathfinder Experiment and James Clerk Maxwell Telescope spectroscopy of the CO 2→1...
ALMA observations have revealed nuclear dusty molecular disks or tori with characteristic sizes 15-4...
In order to investigate circumnuclear molecular gaseous contents and their relation to the nuclear a...