We present CO(1-0) maps of 12 warm H2-selected Hickson Compact Groups (HCGs), covering 14 individually imaged warm H2 bright galaxies, with the Combined Array for Research in Millimeter Astronomy. We found a variety of molecular gas distributions within the HCGs, including regularly rotating disks, bars, rings, tidal tails, and possibly nuclear outflows, though the molecular gas morphologies are more consistent with spirals and early-type galaxies than mergers and interacting systems. Our CO-imaged HCG galaxies, when plotted on the Kennicutt-Schmidt relation, shows star formation (SF) suppression of distributed bimodally, with five objects exhibiting suppressions of 10 and depletion timescales 10 Gyr. This SF inefficiency is also seen in th...
International audienceThe mechanisms governing the stellar mass assembly and star formation history ...
The process by which massive galaxies transition from blue, star-forming disks into red, quiescent g...
Interactions between galaxies have spectacular effects on gas dynamics, and small galaxy groups are ...
We present CO(1–0) maps of 12 warm H_2-selected Hickson Compact Groups (HCGs), covering 14 individua...
Compact groups (CGs) provide an environment in which interactions between galaxies and with the intr...
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transfor...
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transfor...
The physical mechanisms that quench star formation, turning blue star-forming galaxies into red quie...
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transfor...
We present an in depth study on the evolution of galaxy properties in compact groups over the past 3...
One of the greatest challenges to theoretical models of massive galaxy formation is the regulation o...
We present Herschel observations of 22 radio galaxies, selected for the presence of shocked, warm mo...
Star formation is observed to be suppressed in group and cluster galaxies compared to the field. To ...
We present high spatial resolution imaging of the CO(1-0) line from the Karl G. Jansky Very Large Ar...
We present results from a Spitzer mid-infrared spectroscopy study of a sample of 74 galaxies located...
International audienceThe mechanisms governing the stellar mass assembly and star formation history ...
The process by which massive galaxies transition from blue, star-forming disks into red, quiescent g...
Interactions between galaxies have spectacular effects on gas dynamics, and small galaxy groups are ...
We present CO(1–0) maps of 12 warm H_2-selected Hickson Compact Groups (HCGs), covering 14 individua...
Compact groups (CGs) provide an environment in which interactions between galaxies and with the intr...
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transfor...
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transfor...
The physical mechanisms that quench star formation, turning blue star-forming galaxies into red quie...
Context. Galaxies in Hickson Compact Groups (HCGs) are believed to experience morphological transfor...
We present an in depth study on the evolution of galaxy properties in compact groups over the past 3...
One of the greatest challenges to theoretical models of massive galaxy formation is the regulation o...
We present Herschel observations of 22 radio galaxies, selected for the presence of shocked, warm mo...
Star formation is observed to be suppressed in group and cluster galaxies compared to the field. To ...
We present high spatial resolution imaging of the CO(1-0) line from the Karl G. Jansky Very Large Ar...
We present results from a Spitzer mid-infrared spectroscopy study of a sample of 74 galaxies located...
International audienceThe mechanisms governing the stellar mass assembly and star formation history ...
The process by which massive galaxies transition from blue, star-forming disks into red, quiescent g...
Interactions between galaxies have spectacular effects on gas dynamics, and small galaxy groups are ...