Astronomers discover the first hibernating stellar magnet

September 25th, 2008 - 2:12 pm ICT by ANI  

Munich, September 25 (ANI): Astronomers have discovered a most bizarre celestial object that emitted 40 visible-light flashes before becoming dormant again, which might be the first case of a magnetar with an amazingly powerful magnetic field that showed some brief, strong visible-light activity.

This weird object initially misled its discoverers as it showed up as a gamma-ray burst, suggesting the death of a star in the distant Universe.

But soon afterwards, it exhibited some unique behaviour that indicates its origin is much closer to us.

After the initial gamma-ray pulse, there was a three-day period of activity during which 40 visible-light flares were observed, followed by a brief near-infrared flaring episode 11 days later, which was recorded by ESO’’s Very Large Telescope.

Then, the source became dormant again.

We are dealing with an object that has been hibernating for decades before entering a brief period of activity, explained Alberto J. Castro-Tirado, lead author of a research paper that discussed the matter.

The most likely candidate for this mystery object is a magnetar located in our own Milky Way galaxy, about 15 000 light-years away towards the constellation of Vulpecula, the Fox.

Magnetars are young neutron stars with an ultra-strong magnetic field a billion billion times stronger than that of the Earth.

A magnetar would wipe the information from all credit cards on Earth from a distance halfway to the Moon, said co-author Antonio de Ugarte Postigo.

Magnetars remain quiescent for decades. It is likely that there is a considerable population in the Milky Way, although only about a dozen have been identified, he added.

Some scientists have noted that magnetars should be evolving towards a pleasant retirement as their magnetic fields decay, but no suitable source had been identified up to now as evidence for this evolutionary scheme.

The newly discovered object, known as SWIFT J195509+261406 and showing up initially as a gamma-ray burst (GRB 070610), is the first candidate.

The magnetar hypothesis for this object is reinforced by another analysis, based on another set of data. (ANI)

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