In this Letter, we report the discovery of CO fluxes, suggesting very high gas fractions in three disk galaxies seen in the nearby universe (z ∼ 0.1). These galaxies were investigated as part of the DYnamics of Newly Assembled Massive Objects (DYNAMO)
We have resolved molecular gas in a star forming disk galaxy at z>2 down to the scale of ~500 pc. Pr...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
The molecular gas is very difficult to resolve in high-redshift galaxies. Therefore, most of the sur...
In this Letter, we report the discovery of CO fluxes, suggesting very high gas fractions in three di...
In this Letter, we report the discovery of CO fluxes, suggesting very high gas fractions in three di...
We present the first detection of molecular gas cooling CO emission lines from ordinary massive gala...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
Dense molecular clouds are critical to the activity occurring in galactic nuclei. They are the activ...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
We present evidence for very high gas fractions and extended molecular gas reservoirs in normal, nea...
We present Karl G. Jansky Very Large Array observations of the CO(2-1) emission in the z = 4.05 subm...
Abstract We report high-quality Hα/CO imaging spectroscopy of nine massive (log media...
A search for CO(2--1) emission from 42 early type galaxies with 100¯m flux densities greater than 1 ...
We have resolved molecular gas in a star forming disk galaxy at z>2 down to the scale of ~500 pc. Pr...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
The molecular gas is very difficult to resolve in high-redshift galaxies. Therefore, most of the sur...
In this Letter, we report the discovery of CO fluxes, suggesting very high gas fractions in three di...
In this Letter, we report the discovery of CO fluxes, suggesting very high gas fractions in three di...
We present the first detection of molecular gas cooling CO emission lines from ordinary massive gala...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
Dense molecular clouds are critical to the activity occurring in galactic nuclei. They are the activ...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
International audienceWe present evidence for very high gas fractions and extended molecular gas res...
We present evidence for very high gas fractions and extended molecular gas reservoirs in normal, nea...
We present Karl G. Jansky Very Large Array observations of the CO(2-1) emission in the z = 4.05 subm...
Abstract We report high-quality Hα/CO imaging spectroscopy of nine massive (log media...
A search for CO(2--1) emission from 42 early type galaxies with 100¯m flux densities greater than 1 ...
We have resolved molecular gas in a star forming disk galaxy at z>2 down to the scale of ~500 pc. Pr...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
The molecular gas is very difficult to resolve in high-redshift galaxies. Therefore, most of the sur...