CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around
star-forming galaxies at high redshift
CO(1--0) imaging reveals 10-kiloparsec molecular gas reservoirs around
star-forming galaxies at high redshift
Massive, intensely star-forming galaxies at high redshift require a supply of molecular gas from their gas reservoirs, replenished by infall from the surrounding circumgalactic medium, to sustain their immense star-formation rates. However, our knowledge of the extent and morphology of their cold-gas reservoirs is still in its infancy. We present …