‘In these times, during the rise in the popularity of institutional repositories, the Society does not forbid authors from depositing their work in such repositories. However, the AAS regards the deposit of scholarly work in such repositories to be a decision of the individual scholar, as long as the individual's actions respect the diligence of the journals and their reviewers.’ Original article can be found at : http://iopscience.iop.org/ Copyright American Astronomical SocietyThermal 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 × 107 M ring of dense and cold clouds orbiting the Galactic center. Using a simple toy model, an elliptica...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We assess a claim that observed galaxy clusters with mass ∼1014M⊙ are more centrally concentrated th...
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...
International audienceThermal images of cold dust in the Central Molecular Zone of the Milky Way, ob...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
Panchromatic observations of the best candidate hyperluminous infrared galaxies from the widest Hers...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
Large-scale structures (LSSs) out to z 0.8, the SFR density is uniformly distributed over all envir...
The Orion Molecular Complex is the nearest site of ongoing high-mass star formation, making it one o...
Extreme emission line galaxies (EELGs) are considered the primary contributor to cosmic reionization...
We have discovered a 300 kpc-wide giant Lyman-α (Lyα) nebula centered on the massive galaxy group RO...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We assess a claim that observed galaxy clusters with mass ∼1014M⊙ are more centrally concentrated th...
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...
International audienceThermal images of cold dust in the Central Molecular Zone of the Milky Way, ob...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
Panchromatic observations of the best candidate hyperluminous infrared galaxies from the widest Hers...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
Large-scale structures (LSSs) out to z 0.8, the SFR density is uniformly distributed over all envir...
The Orion Molecular Complex is the nearest site of ongoing high-mass star formation, making it one o...
Extreme emission line galaxies (EELGs) are considered the primary contributor to cosmic reionization...
We have discovered a 300 kpc-wide giant Lyman-α (Lyα) nebula centered on the massive galaxy group RO...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
‘In these times, during the rise in the popularity of institutional repositories, the Society does n...
We assess a claim that observed galaxy clusters with mass ∼1014M⊙ are more centrally concentrated th...