Galaxy mergers—wherein 2 galaxies combine together during the course of billions of years in at times-striking bursts of light—are not always simple for astronomers to notice. Now, researchers from the University of Colorado Boulder have built a new method for discovering these cosmic couplings in examinations of the night sky.
In the latest study, a team directed by Rebecca Nevin developed a computer program that scrutinizes through examinations of galaxies to seek a broad array of indications that a merger might be taking place. That comprises the resulting galaxies’ shape and how the stars within are stirring. That’s significant, Nevin said, as such mergers might be a vital step in the developing of enormous, spiral galaxies such as the Milky Way and in stimulating the new stars’ formation.
An Assistant Prof. at the University of Florida who directed the simulation work, Laura Blecha, said, “These simulated galaxy unions permit us to directly trail billions of years of development, while examinations of actual galaxies are restricted to single instants in time.” The scientists utilized those simulations to tutor a computer program to identify the revealing fingerprints of these mergers. Then the group—that comprised Jenny Greene from the Princeton University and Julia Comerford from CU Boulder—used the identical program to scrutinize real-life pictures of galaxies gathered by the SDSS.
And it worked: based on the sorts of galaxies entailed the team’s method could accurately recognize merging galaxies 80% of the time or more.
Likewise, we know a supermassive black hole exists at our Milky Way galaxy’s center. However, as per a recent study, it appears that few of these supermassive black holes have observed d unexpected growth spurts during which they speedily consume enormous amounts of gases from the nearby region. Earlier, no such growth spurts were been spotted ever and this new discovery could help researchers get a better comprehension of how galaxies such as ours formed.