HST images of extreme cases of ram-pressure stripping in galaxy clusters at z > 0:2. From left to right: galaxy C153 in A2125 at z = 0:20 (WFPC2, F606W+F814W, Owen et al. 2006); galaxy 234144–260358 in A2667 at z = 0:23 (ACS, F450W+F606W+F814W, Cortese et al. 2007); galaxy F0083 in A2744 at z = 0:31 (ACS, F435W+F606W+F814W, Owers et al. 2012). Credit: arXiv:1312.6135 [astro-ph.CO]
(Phys.org) —A trio of researchers, two from the University of Hawaii, and one from the University of Dunham in the U.K. has found evidence from the Hubble Space Telescope that suggests jellyfish galaxies come about when spiral galaxies are ripped apart as they move towards dense galaxy clusters. In their paper published in The Astrophysical Journal Letters, the team describes how six images of jellyfish captured by Hubble appear to show how spiral galaxies morph into elliptical galaxies.
Prior research has shown that in dense parts of the galaxy, elliptical galaxies tend to outnumber spiral galaxies—likely due, some have suggested, to some unknown transformation process. In this new effort, the researchers suggest that the mysterious transformation process appears to come about as spiral galaxies encounter the enormous heat present in dense galaxy clusters.
Dense galaxy clusters are thought to come about due to happenstance arrangement of galaxies—those that are close enough to others, draw ever closer to each other due to gravity—as the area of space grows more dense the gasses between the galaxies grows hotter. Anything that approaches the dense area is impacted by the heated gas.
In studying images captured by Hubble, the researchers have witnessed what they believe to be the process by which galaxies evolve in such dense parts of space. They believe that when a spiral galaxy nears a dense galaxy cluster, its colder gases tend to get pulled in to the cluster, causing a stretching of the spiral, and resulting in what is known as a jellyfish galaxy—so named because of its resemblance to the sea creature. Stars from the outer edges of the spiral galaxy are pulled into the cluster, wrecking its signature shape. Over time, the entire spiral galaxy is pulled into the cluster where it melds with other galaxies to form an elliptical galaxy.
The new theory explains both the presence of jellyfish galaxies and so-named orphan stars that don't appear to exist as part of any galaxy—they're actually in transit, the researchers believe, after being pulled from a spiral—eventually they'll wind up as part of an elliptical galaxy.
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