International audienceThermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-infrared cameras on board the Herschel satellite, reveal a similar to 3 x 10(7) M-circle dot ring of dense and cold clouds orbiting the Galactic center. Using a simple toy model, an elliptical shape having semi-major axes of 100 and 60 pc is deduced. The major axis of this 100 pc ring is inclined by about 40 degrees with respect to the plane of the sky and is oriented perpendicular to the major axes of the Galactic Bar. The 100 pc ring appears to trace the system of stable x(2) orbits predicted for the barred Galactic potential. Sgr A* is displaced with respect to the geometrical center of symmetry of the ring. The ring is...
We show that in the anticenter region, between Galactic longitudes of 110 degrees < l < 229 de...
Most of the Galactic center (GC) gas moves in nearly circular orbits in a nuclear ring (hereafter th...
International audienceABSTRACT Using analytic modelling and simulations, we address the origin of an...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
We present 19.7, 31.5, and 37.1 µm images of the inner 6 pc of the Galactic Center of the Milky Way ...
We derive the physical properties of 580 molecular clouds based on their (12)CO and (13)CO line emis...
The 4.6m millimeter wave telescope at the University of British Columbia has been used to map a regi...
A model is proposed in which most of the molecular clouds near the galactic center are situated in a...
Context. Ring-like structures in the interstellar medium (ISM) are commonly associated with high-mas...
International audienceContext. Dusty debris discs around main sequence stars are thought to be the r...
We compile position and inclination angles for tilted ring fits to the warped dusty and gaseous disk...
We show that in the anticenter region, between Galactic longitudes of 110 degrees < l < 229 de...
Most of the Galactic center (GC) gas moves in nearly circular orbits in a nuclear ring (hereafter th...
International audienceABSTRACT Using analytic modelling and simulations, we address the origin of an...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
We present 19.7, 31.5, and 37.1 µm images of the inner 6 pc of the Galactic Center of the Milky Way ...
We derive the physical properties of 580 molecular clouds based on their (12)CO and (13)CO line emis...
The 4.6m millimeter wave telescope at the University of British Columbia has been used to map a regi...
A model is proposed in which most of the molecular clouds near the galactic center are situated in a...
Context. Ring-like structures in the interstellar medium (ISM) are commonly associated with high-mas...
International audienceContext. Dusty debris discs around main sequence stars are thought to be the r...
We compile position and inclination angles for tilted ring fits to the warped dusty and gaseous disk...
We show that in the anticenter region, between Galactic longitudes of 110 degrees < l < 229 de...
Most of the Galactic center (GC) gas moves in nearly circular orbits in a nuclear ring (hereafter th...
International audienceABSTRACT Using analytic modelling and simulations, we address the origin of an...