XMM-Newton measures speedy spin of rare celestial object

January 14th, 2009 - 3:19 pm ICT by ANI  

Paris, Jan 14 (ANI): The XMM-Newton telescope has captured the fading glow of a tiny and rare celestial object, revealing its rotation rate for the first time.

The new information confirms this particular object as one of an extremely rare class of stellar zombie each one the dead heart of a star that refuses to die.

There are just five so-called Soft Gamma-ray Repeaters (SGRs) known, four in the Milky Way and one in our satellite galaxy, the Large Magellanic Cloud.

Each is between 10 and 30 km across, yet contains about twice the mass of the Sun. Each one is the collapsed core of a large star that has exploded, collectively called neutron stars.

What sets the Soft Gamma-ray Repeaters apart from other neutron stars is that they possess magnetic fields that are up to 1000 times stronger. This has led astronomers to call them magnetars.

SGR 1627-41 was discovered in 1998 by NASAs Compton Gamma Ray Observatory when it burst into life emitting around a hundred short flares during a six-week period. It then faded before X-ray telescopes could measure its rotation rate.

Thus, SGR 1627-41 was the only magnetar with an unknown period.

Last summer, SGR 1627-41 flared back into life. But, it was located in a region of sky that ESAs XMM-Newton was unable to point at for another four months.

This was because XMM-Newton has to keep its solar panels turned towards the Sun for power.

So, astronomers waited until Earth moved along its orbit, carrying XMM-Newton with it and bringing the object into view.

During that time, SGR 1627-41 began fading fast.

When it came into view in September 2008, thanks to the superior sensitivity of the EPIC instrument on XMM-Newton, it was still detectable.

A team of astronomers took the necessary observations and revealed that it rotates once every 2.6 seconds.

This makes it the second fastest rotating magnetar known, said Sandro Mereghetti from the research team.

With a rotation rate of 2.6 seconds, this magnetar must be old enough to have slowed down. Another clue to the magnetars age is that it is still surrounded by a supernova remnant.

During the measurement of its rotation rate, XMM-Newton also detected X-rays coming from the debris of an exploded star, possibly the same one that created the magnetar.

These usually fade to invisibility after a few tens of thousand years. The fact that we still see this one means it is probably only a few thousand years old, said Mereghetti. (ANI)

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