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Explosion Reveals Tiny Magnetic Island

Magnetars are perplexing objects.
by Staff Writers
Paris, France (ESA) Sep 21, 2007
ESA's XMM-Newton, has provided new insight into puzzling celestial objects known as magnetars. Thanks to the orbiting X-ray observatory, astronomers have traced powerful explosions to a region just beneath a magnetar's surface. Magnetars are small neutron stars that occasionally suffer extraordinarily powerful outbursts which shine X-rays across the galaxy. In 2003, astronomers saw a neutron star brighten to around 100 times its usual faint luminosity.

This outburst allowed them to discover XTE J1810-197. Detecting pulsations from the source helped classify it as the first transient anomalous X-ray pulsar (AXP). The massive outburst moved it to the rank of magnetar.

Magnetars are perplexing objects. Each one is the highly magnetic core of a star that was once at least eight times more massive than the Sun. When it exploded as a supernova, the core was compressed into a highly compact object, a neutron star, roughly fifteen kilometres in diameter, but containing about as much mass as the Sun.

Some of these neutron stars possess the most powerful magnetic fields in the Universe, leading to extremely energetic eruptions that send high-energy radiation cascading across space. Astronomers have never been certain whether the outbursts come from the surface of the magnetar itself, or the clouds of electrically charged particles trapped in the surrounding magnetic field.

Now, using data from XMM-Newton, Tolga Guver, Istanbul University, and his colleagues have analysed the X-ray spectrum of XTE J1810-197 using a computer model that incorporates emission from the magnetar's surface with its subsequent processing as it travels through the object's magnetic field. This is the first time both regions of a magnetar have been put together in the same computer model.

XMM-Newton observed XTE J1810-197 seven times between 9 August 2003 and 12 March 2006 using XMM's European Photon Imaging Camera (EPIC) on board XMM. During that time, the object faded back to normal brightness, and EPIC recorded the changes in the energies of the X-rays released as it did so. These changes are particularly valuable to astronomers because they can be compared with computer predictions.

Guver and colleagues found that the data were best fitted with a model that traced the outburst to just below the surface of the magnetar and confined it to an area about 3.5 km across. This is a breakthrough because, "Assuming our model is confirmed, we can now distinguish between surface and magnetopheric phenomena," says Guver.

Their model also allowed them to determine the strength of this object's magnetic field spectroscopically. It is around six hundred million, million times stronger than Earth's magnetic field. Encouragingly, this measurement is similar to an estimate made previously for this object based on how fast its spin is slowing down. This boosts the team's confidence that their model is correct.

Nevertheless, they are not being complacent about their work. "This model will not be the final one about magnetars but it does give us a new point of view onto these fascinating objects," says Guver.

One thing that remains unclear is the nature of the outburst. It is probably triggered magnetically but exactly how, is still a mystery. The team now plan to use their computer model to investigate more of these celestial objects, using more data from XMM-Newton, in their quest for answers.

'The Magnetar Nature and the Outburst Mechanism of a Transient Anomalous X-ray Pulsar' by T. Guver, F. Özel, E. Gogus and C. Kouveliotou is due to be published in The Astrophysical Journal, on 20 September 2007.

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'Orphan' Stars Found In Long Galaxy Tail
Huntsville AL (SPX) Sep 21, 2007
Astronomers have found evidence that stars have been forming in a long tail of gas that extends well outside its parent galaxy. This discovery suggests that such "orphan" stars may be much more prevalent than previously thought. The comet-like tail was observed in X-ray light with NASA's Chandra X-ray Observatory and in optical light with the Southern Astrophysical Research (SOAR) telescope in Chile. The feature extends for more than 200,000 light years and was created as gas was stripped from a galaxy called ESO 137-001 that is plunging toward the center of Abell 3627, a giant cluster of galaxies.







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