Like a pixie trailing fairy dust that makes flowers bloom, a lone galaxy is shedding gas that's forming stars as it plunges toward the center of a massive galaxy cluster.
Ming Sun, Megan Donahue, and Mark Voit of Michigan State University found the tail of stars using the 4.1-meter Southern Astrophysical Research (SOAR) telescope in Chile and NASA's Chandra X-ray Observatory. The composite visible-light / X-ray image at right shows the tail spanning more than 200,000 light-years.
The speedy galaxy, dubbed ESO 137-001, is located in the cluster Abell 3627 more than 200 million light-years away in Triangulum Australe.
The astronomers counted 29 regions of glowing hydrogen gas — indicative of star-forming regions — near the galaxy, all of which lie "downstream."
"This isn't the first time that stars have been seen to form between galaxies," explains Donahue. "But the amount of stars forming here is unprecedented." It's unusual for gas escaping a galaxy to be dense enough to allow stars to coalesce on their own.
For more details, see the NASA press release or the full paper to be published in the Astrophysical Journal in December.
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