Thermal 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 ~3 × 10^7 M_☉ 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° 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 twisted and its morphology suggests a flattening ...
We present Herschel-SPIRE observations at 250–500 μm of the giant elliptical galaxy M 86 and examine...
We present evidence that the curious stellar population found by the Sloan Digital Sky Survey in the...
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...
International audienceThermal images of cold dust in the Central Molecular Zone of the Milky Way, ob...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
We present hydrodynamic simulations of gas clouds in the central kpc region of the Milky Way that is...
We use hydrodynamical simulations to study the Milky Way’s central molecular zone (CMZ). The simulat...
The Galactic center hosts several hundred early-type stars, about 20% of which lie in the so-called ...
We present 19.7, 31.5, and 37.1 µm images of the inner 6 pc of the Galactic Center of the Milky Way ...
Using photometry of NGC 1097 from the Herschel PACS (Photodetector Array Camera and Spectrometer) in...
A model is proposed in which most of the molecular clouds near the galactic center are situated in a...
Using photometry of NGC 1097 from the Herschel PACS (Photodetector Array Camera and Spectrometer) in...
We present Herschel-SPIRE observations at 250–500 μm of the giant elliptical galaxy M 86 and examine...
We present evidence that the curious stellar population found by the Sloan Digital Sky Survey in the...
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...
International audienceThermal images of cold dust in the Central Molecular Zone of the Milky Way, ob...
Thermal images of cold dust in the Central Molecular Zone of the Milky Way, obtained with the far-in...
We present hydrodynamic simulations of gas clouds in the central kpc region of the Milky Way that is...
We use hydrodynamical simulations to study the Milky Way’s central molecular zone (CMZ). The simulat...
The Galactic center hosts several hundred early-type stars, about 20% of which lie in the so-called ...
We present 19.7, 31.5, and 37.1 µm images of the inner 6 pc of the Galactic Center of the Milky Way ...
Using photometry of NGC 1097 from the Herschel PACS (Photodetector Array Camera and Spectrometer) in...
A model is proposed in which most of the molecular clouds near the galactic center are situated in a...
Using photometry of NGC 1097 from the Herschel PACS (Photodetector Array Camera and Spectrometer) in...
We present Herschel-SPIRE observations at 250–500 μm of the giant elliptical galaxy M 86 and examine...
We present evidence that the curious stellar population found by the Sloan Digital Sky Survey in the...
International audienceABSTRACT Using analytic modelling and simulations, we address the origin of an...