Astronomers baffled by 'super fast star'

thecheers.org    2008-05-17 02:07:55    


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Canberra, May 17 : Astronomers have been baffled by the discovery of a star that lies 20,000 light-years away, spinning at a rate of 465 revolutions per second - the fifth fastest-spinning pulsar known in our Galaxy. The super fast pulsar, called J1903+0327, was detected with the Arecibo radio telescope in Puerto Rico.

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Astronomers have been baffled by the discovery of a star that lies 20,000 light-years away, spinning at a rate of 465 revolutions per second - the fifth fastest-spinning pulsar known in our Galaxy.
The super fast pulsar, called J1903+0327, was detected with the Arecibo radio telescope in Puerto Rico.

Astronomers believe such super-fast pulsars started life as the more common, sedate pulsars that spin only a few times a second, but were later 'reborn' in their present hyperactive state.

According to astronomers, this re-birthing or recycling can take place if the pulsar has a nearby companion that it orbits. At a certain point in its life cycle, the companion pours its own matter onto the pulsar and this extra material 'spins-up' the pulsar.

The process makes the pulsar's orbit around its companion almost completely circular, or as astronomers put it, the orbit has "low eccentricity".

"This low eccentricity is one of the best pieces of evidence we have for recycling theory," said Dr Champion from CSIRO's Australia Telescope National Facility. "But J1903+0327 is totally different in that it has a very eccentric orbit which is elliptical rather than circular," he added.

For astronomers, the mystery is that how did such a star form.

One theory is that the pulsar may once have been part of a triple system of stars and was 'spun-up' by its closest companion star, which was either ejected from the system or worn away after it transferred all its mass to the pulsar.

It might now remain in an elongated orbit around the third, more distant member of the original trio.

But another possible explanation for the pulsar's odd combination of properties is that it was born in a dense region of stars called a globular cluster, and spun-up by its original partner.

As well as having a highly eccentric orbit, the pulsar is heavier than normal with a mass of about 1.74 times that of the Sun. "A pulsar this massive could also rule out some theories about the state of the highly compressed matter in pulsars," said Dr Champion.

According to Dr Champion, "Pulsars like this are why you do these surveys. You don't want to just find hundreds of objects, you want to find the two or three that are plain weird and we've found one." (ANI)
© 2007 ANI

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