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Spinning Galactic Tails
     August 8, 2003
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When Stars Collide

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Spinning Galactic Tails 

EMBARGOED for

Given the headline, you might expect that the large, disrupted galaxy with the long tail is the subject of this Image of the Day. The chaotic Tadpole Galaxy, photographed last year by the Hubble Space Telescope, is actually one tiny blue galaxy almost entirely consumed by another larger one and generating the tail of stars.

The Tadpole, however, is not in the news today. But it does sort of relate to the final chapter of a story told by another pair of galaxies in the image.

Astronomers found something interesting going on with the bright spiral galaxy that sits, tilted at an angle, near the lower left of the image.

The spiral, which looks comparatively small here, is farther away than the Tadpole and so is actually of a common, standard size. It, too, has a companion galaxy, one called a dwarf that it has just begun consuming. Tethering the two is a stream of stars pulled out from the dwarf companion by the spiral galaxy's more powerful gravity.

You can't see the faint stream of stars in the main image, but it's visible in this close-up (in which the spiral galaxy has been tilted a different direction by the researchers, perhaps just to confuse you). The stream was enhanced through computer modeling to make it even more apparent (and you can see that stuff here).

The scene is cited as evidence for galaxy gobbling, and it is one of the earliest stages of the process ever photographed.

"Although long predicted, direct evidence for plumes of stars being ripped from a dwarf galaxy as it is swallowed up by a giant galaxy has remained elusive," said Duncan Forbes, an astronomer at Swinburne University of Technology in Australia who led the investigation. "This discovery provides the best evidence to date,"

Our own Milky Way Galaxy is thought to have built its bulk in part by swallowing smaller galaxies, and it is still doing so. The new study was detailed yesterday in the online version of the journal Science.

-- Robert Roy Britt

Credit: Hubble, STScI, Swinburne University of Technology



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