Washington: NASA’s Rossi X-ray Timing Explorer (RXTE) has captured the month-long fusillade of a unique neutron star near the centre of our galaxy erupting with hundreds of X-ray bursts, that were powered by a barrage of thermonuclear explosions its surface, in extreme detail.
A neutron star is the closest thing to a black hole that astronomers can observe directly, crushing half a million times more mass than Earth into a sphere no larger than a city.
Using this data from the star burst in October 2010, an international team of astronomers has been able to bridge a long-standing gap between theory and observation.
“In a single month from this unique system, we have identified behavior not seen in observations of nearly 100 bursting neutron stars during the past 30 years,” Manuel Linares, the study leader from Massachusetts Institute of Technology in Cambridge, said.
This graph based on RXTE data provides an overview of the changing character of T5X2’s X-ray emission during outbursts from Oct. 13 to Nov. 19, 2010.
As the persistent X-ray emission rises, the burst rate increases while the burst brightness decreases. The abrupt dropout on October 13 occurred when the moon briefly covered the source.
On Oct. 10, 2010, the European Space Agency’s INTEGRAL satellite detected a transient X-ray source in the direction of Terzan 5, a globular star cluster about 25,000 light-years away toward the constellation Sagittarius.
The object, dubbed IGR J17480–2446, is classed as a low-mass X-ray binary system, in which the neutron star orbits a star much like the sun and draws a stream of matter from it. As only the second bright X-ray source to be found in the cluster, Linares and his colleagues shortened its moniker to T5X2.
Three days after the source’s discovery, RXTE targeted T5X2 and detected regular pulses in its emission, indicating that the object was a pulsar -- a type of neutron star that emits electromagnetic energy at periodic intervals.
The object’s powerful magnetic field directs infalling gas onto the star’s magnetic poles, producing hot spots that rotate with the neutron star and give rise to X-ray pulses.
At NASA’s Goddard Space Flight Center in Greenbelt, Md., RXTE scientists Tod Strohmayer and Craig Markwardt showed that T5X2 spins at a sedate -- for neutron stars -- rate of 11 times a second. And because the pulsar’s orbital motion imparts small but regular changes in the pulse frequency, they showed that the pulsar and its sun-like companion revolve around each other every 21 hours.
This illustration compares the size of a neutron star to Manhattan. The crushed core of a star that has exploded as a supernova, a neutron star packs more mass than the sun into a sphere just 10 to 15 miles wide.
That same day, RXTE observed its first burst from the system: an intense spike in X-rays lasting nearly 3 minutes and caused by a thermonuclear explosion on the neutron star``s surface. Ultimately, RXTE catalogued some 400 events like this between Oct. 13 and Nov. 19, with additional bursts observed by INTEGRAL and NASA’s Swift and Chandra observatories. NASA decommissioned RXTE on Jan. 5, 2012.
In the T5X2 system, matter streams from the sun-like star to the neutron star, a process called accretion. Because a neutron star packs more than the sun’s mass into a sphere between 10 and 15 miles across -- about the size of Manhattan or the District of Columbia -- its surface gravity is extremely high.
The gas rains onto the pulsar’s surface with incredible force and ultimately coats the neutron star in a layer of hydrogen and helium fuel. When the layer builds to a certain depth, the fuel undergoes a runaway thermonuclear reaction and explodes, creating intense X-ray spikes detected by RXTE and other spacecraft.
The bigger the blast, the more intense its X-ray emission.
Models designed to explain these processes made one prediction that had never been confirmed by observation. At the highest rates of accretion, they said, the flow of fuel onto the neutron star can support continuous and stable thermonuclear reactions without building up and triggering episodic explosions.
Terzan 5, which hosts the T5X2 system, is a dense globular star cluster located 25,000 light-years away toward the constellation Sagittarius.
At low rates of accretion, T5X2 displays the familiar X-ray pattern of fuel build-up and explosion: a strong spike of emission followed by a long lull as the fuel layer reforms. At higher accretion rates, where a greater volume of gas is falling onto the star, the character of the pattern changes – the emission spikes are smaller and occur more often.
But at the highest rates, the strong spikes disappeared and the pattern transformed into gentle waves of emission. Linares and his colleagues interpret this as a sign of marginally stable nuclear fusion, where the reactions take place evenly throughout the fuel layer, just as theory predicted.
“We see T5X2 as a ‘model burster,’ the one that’s doing everything expected of it,” Diego Altamirano, co-author of the paper from the University of Amsterdam in The Netherlands, said.
The study will be published in The Astrophysical Journal.