A Spectroscopically Confirmed Excess of 24 μm Sources in a Super Galaxy Group at z=0.37: Enhanced Dusty Star Formation Relative to the Cluster and Field Environment
Stefan Kautsch
Part of the Physical Sciences and Mathematics Commons
Part of the Physical Sciences and Mathematics Commons
A Spectroscopically Confirmed Excess of 24 μm Sources in a Super Galaxy Group at z=0.37: Enhanced Dusty Star Formation Relative to the Cluster and Field Environment
Stefan Kautsch