... passed the cluster core, the direction of motion of the clustergas reversed, and it traveled back toward the cluster center ... The clustergas moved through the center again and т??sloshedт?? back and forth. ...
... roughly 100 solar masses of gas before the cluster crosses the galactic plane ... At that time, gas in the Milky Way's plane hits clustergas and removes it. ... if the star were in a globular cluster, its gas would quickly escape the cluster's ...
... determined the ratio of the cluster's gas mass to its total mass, including dark ... problem, researchers had to understand the distribution of hot gas in the cluster ...
... is the pressure of the cluster's hot gas plasma, reaching temperatures as high as 10 ... from the action of the hot clustergas resemble those affecting comets in our Solar ...
... which blows bubbles of radio-wave emitting material into the surrounding clustergas ... relationship between the central black hole and the surrounding clustergas ... of the complex interaction between the clustergas and the supermassive black hole ...
... amount of iron contained in the gas filling the cluster amounts to 50 billion times ... New gas entering the cluster falls toward its center, eventually moving fast enough ...
... analysis of the HST images and the clustergas distribution (red) based on Chandra X ... and become stuck between the clusters, making a huge cloud of gas a thousand times ...
... s enough turbulence in galaxy clusters to keep gas from cooling and forming new ... Over time, the gas in the centers of these clusters should cool enough that stars ...
... the rate of hot gas cooling in the central regions of the cluster is the largest ... a cluster are apparently not powerful enough to prevent the clustergas from cooling ...
... Overlaid on the Hubble Space Telescope (HST) color image of the galaxies is the total mass distribution (blue) based on WL analysis of the HST images and the clustergas distribution (red) based on Chandra X-ray observations. ...