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Nov. 8, 2010
Courtesy of the University of Portsmouth
and World Science staff
Courtesy of the University of Portsmouth
and World Science staff
Helped by an army of citizen volunteers, scientists have concluded that bar-like structures found in many spiral galaxies—including our own—could be helping to destroy their graceful, twisty forms.
Most stars are part of galaxies, vast groupings of stars containing from a few hundred million to a quadrillion of the fiery balls. Galaxies themselves come in many shapes, including elliptical (watermellon-shaped) and irregular. Others are majestic spirals in which spiral "arms" formed by stars and other material wind out in a disk from a central bulge.
Most stars are part of galaxies, vast groupings of stars containing from a few hundred million to a quadrillion of the fiery balls. Galaxies themselves come in many shapes, including elliptical (watermellon-shaped) and irregular. Others are majestic spirals in which spiral "arms" formed by stars and other material wind out in a disk from a central bulge.
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| A barred spiral galaxy, NGC 3351. (Credit: NASA |
Bars are believed to strongly influence the evolution of galaxies as they provide a way to move material in and out in the disk and possibly help to spark star formation in the central regions. They may even help feed the central massive black hole that seems to be present in almost all galaxies.
But scientists don't understand why some galaxies have bars and others don't.
In the new study, scientists drew on the work of volunteers for Galaxy Zoo 2, an online project in which members of the public are asked to carefully classify galaxies shown in photos.
With these data — which they called the largest ever sample of galaxies with visual bar identifications — the researchers, led by cosmologist Karen Masters at the University of Portsmouth in the U.K., determined that reddish spirals are about twice as likely to host bars as bluish spirals. This matters because color is a clue to galaxy age. "Blue" galaxies get their hue from the hot young stars they contain, implying that they are forming many stars and are young. In "red" galaxies, this star formation has stopped, leaving behind the cooler, long-lived stars, which are redder.
The astronomers conclude that bars might help to kill spiral galaxies, although how they do it remains a mystery. But the Milky Way has a bar too, so the finding may be telling us something about its future.
In a statement issued as the findings were revealed this week, Masters wasn't focusing on any dismay she might feel for the possible aesthetic demise of our home galaxy. Instead, she said it was "wonderful" to have "so many people involved in this research."
"I feel a great weight of responsibility to make sure good science comes out of all the hard work they put into classifying galaxies," she added. Data hinting at the new result has existed for "some time," she went on, but "with such a large number of bar classifications we're much more confident about our results. And all of this is thanks to the dedication of the volunteers who provide the raw 'clicks'.
"It's not yet clear whether the bars are some side effect of an external process that turns spiral galaxies red, or if they alone can cause this transformation. We should get closer to answering that question with more work on the Galaxy Zoo dataset."
A paper on the findings is to appear in the journal Monthly Notices of the Royal Astronomical Society and is also posted on the online database arXiv.org.
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Source: http://basistik.blogspot.com/2011/06/universal-physics-bars-may-kill-spiral.html
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