XMM-Newton finds the leader of the Magnificent Seven in a spin (Forwarded)

ESA News
http://www.esa.int

9 March 2007

XMM-Newton finds the leader of the Magnificent Seven in a spin

A decade-long mystery has been solved using data from ESA's X-ray
observatory XMM-Newton. The brightest member of the so-called 'magnificent
seven' has been found to pulsate with a period of seven seconds.

The discovery casts some doubt on the recent interpretation that this
object is a highly exotic celestial object known as a quark star.

The magnificent seven is a collection of young neutron stars. Neutron
stars are the dead hearts of once massive stars. They contain about 1.4
times the mass of the Sun but are compressed by gravity into ultra-dense
spheres just 10­15 kilometres in diameter. A one Euro coin made of neutron
star material would weigh more than the entire population of Earth. What
sets the magnificent seven apart from the 1700 other neutron stars seen as
radio pulsars is that they are not detected at radio frequencies but their
surfaces are hot enough to emit X-rays.

The brightest member of the magnificent seven, RXJ1856 had been a mystery
to astronomers since its discovery a decade ago because, despite the fact
that it is so bright, no one had been able to find any pulsations and thus
determine its rotation rate. That has all changed thanks to the work of
Andrea Tiengo and Sandro Mereghetti, Istituto Nazionale di Astrofisica,
Milan, Italy.

Using data collected by XMM-Newton, the pair searched for any signs of the
long-sought-after pulsations in RXJ1856. They were successful, finding a
repeating 7-second pulsation over a 19-hour observation of the source
performed in October 2006. They checked other archival data and confirmed
the pulsation registered in five other XMM-Newton observations performed
between 2002 and 2006.

"The pulsations are a typical characteristic of a neutron star," says
Tiengo. It means that the tiny object is spinning and that a hot spot on
its surface is rotating into our line of vision every seven seconds, in
the same way that a lighthouse sweeps its beam of light around in a
circle. The pulsations in RXJ1856 have very low amplitude; this explains
why they were not seen before.

RXJ1856 is an intriguing object for astronomers. The Hubble Space
Telescope has supplied a very accurate distance to the object: 500 light
years. This has allowed astronomers to use the brightness of RXJ1856 to
estimate its radius. What they found puzzled them. The estimated radius
came out to be smaller than 10 kilometres. This was taken as possible
evidence that RXJ1856 was an even more exotic object, known as a quark
star. In such an object, gravity has crushed the atomic nuclei into their
constituent quarks.

"We don't rule out the quark star interpretation but the pulsations show
that the object is also consistent with neutron star models," says Tiengo.

So astronomers are going to have to work harder to determine in which of
these exotic categories RXJ1856 belongs. "If we can obtain more precise
measurements of the period we can then see how fast the object is slowing
down," says Mereghetti.

Neutron stars slow down because their strong magnetic fields (one million,
million times larger than the Earth's field) and fast rotation, produce
electromagnetic radiation that drains their rotational energy. Measuring
the deceleration of the object would give astronomers a clue about its
magnetic field, which is responsible for creating the hot spot that
produces the pulsation.

Note for editors:

The findings will appear in the 10 March 2007 issue of The Astrophysical
Journal, (657: L101­L104, 10 March 2007), in the article by Andrea Tiengo
and Sandro Mereghetti (INAF­Istituto di Astrofisica Spaziale e Fisica
Cosmica, Milan, Italy) titled: "XMM-NEWTON discovery of 7s pulsations in
the isolated neutron star RX J1856.5-3754."

For more information:

Andrea Tiengo
INAF­Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan, Italy
Email: tiengo @ iasf-milano.inaf.it

Sandro Mereghetti
INAF­Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan, Italy
Email: sandro @ iasf-milano.inaf.it

Norbert Schartel
ESA XMM-Newton Project Scientist
Email: norbert.schartel @ sciops.esa.int

[NOTE: Images and weblinks supporting this release are available at
http://www.esa.int/esaCP/SEM1WRN0LYE_index_1.html ]


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