New Data about Galaxy Collision and Merger Rate

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According to new analysis of Hubble surveys, combined with simulations of galaxy interactions, the merger rate of galaxies over the last 8 billion to 9 billion years falls between the previous estimates. The galaxy merger rate is one of the fundamental measures of galaxy evolution, yielding clues to how galaxies bulked up over time through encounters with other galaxies. But there is a huge discrepancy over how often galaxies coalesced in the past. Measurements of galaxies in deep-field surveys made by NASA’s Hubble Space Telescope generated a broad range of results: anywhere from 5 percent to 25 percent of the galaxies were merging. 
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The study, led by Jennifer Lotz of the Space Telescope Science  Institute  in  Baltimore,  Md.,  analyzed  galaxy interactions at different distances, allowing the astronomrs to compare mergers over time. So astronomers could find that galaxies gained quite a bit of mass through collisions with other galaxies. Large galaxies merged with each other on average once over the past 9 billion years. Small galaxies were coalescing with large galaxies more frequently. According to Lotz having an accurate value for the merger rate is critical because galactic collisions may be a key process that drives galaxy assembly, rapid star formation at early times, and the accretion of gas onto central supermassive black holes at the centers of galaxies.