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Cosmic Crumbs Reveal Umbrella Galaxy's 'Cannibalistic' Habits

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GALAXY CANNIBAL
The Umbrella Galaxy was named after the wispy feature seen on the left here that looks like a cosmic parasol. This "umbrella" is actually debris from a small galaxy that has been shredded apart by gravity. This image combines data from the 0.5-metre BlackBird Remote Observatory Telescope and Suprime-Cam on the 8-meter Subaru Telescope in Hawaii. | R. J. GaBany/Blackbird Obs.

Astronomers are studying the feeding habits of a cosmic cannibal to learn how galaxies grow.

If you point a telescope near the constellations of Leo and Virgo, you might be able to catch a glimpse of the galactic monster in question: the Umbrella Galaxy, formally called NGC 4651.

This spiral galaxy — a twin of the Milky Way — is eating a smaller galaxy, and it gets its whimsical nickname from the wispy "parasol" that surrounds it.

When scientists discovered this umbrella in the 1950s, they interpreted it as a dwarf galaxy companion to the bigger galaxy. But recent research has suggested this parasol might actually be made up of crumbs from a leftover meal.

Astronomers have shown that our own Milky Way has fattened up by acquiring stars from other, smaller galaxies. They've found streams of star crumbs emanating from the nearby Sagittarius dwarf galaxy, which is being engulfed by the Milky Way.

What's more, a study in 2010 that looked at eight spiral galaxies, including the Umbrella Galaxy, found that six of them had signs of mergers: shells, clouds and arcs of tidal debris.

Researchers led by Caroline Foster of the Australian Astronomical Observatory (AAO) have been studying the Umbrella Galaxy, and they learned that its distinctive arc is made up of the crumbs from a single dinner, rather than a series of meals.

"Through new techniques we have been able to measure the movements of the stars in the very distant, very faint, stellar stream in the Umbrella," Foster explained in a statement from the AAO. "This allows us to reconstruct the history of the system, which we couldn't before."

The astronomers used observations from the Subaru and Keck telescopes in Hawaii, and they tracked the movement of the stars in the stream by looking at globular clusters, planetary nebulae and patches of hydrogen gas in the galaxy. (Its distance from Earth is not well established, but the researchers in the study estimated that it is 62 million light-years away.)

The study, which has been accepted for publication in the Monthly Notices of the Royal Astronomical Society, is free to read online at the preprint service arxiv.

Follow Megan Gannon on Twitter and Google+. Follow us @Spacedotcom, Facebook or Google+. Originally published on Space.com.

Copyright 2014 SPACE.com, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

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