Astronomers have detected radio jets belonging to a neutron star with a strong magnetic field — something not predicted by current theory, according to a new study published in Nature. The team, led by researchers at the University of Amsterdam, observed the object known as Swift J0243.6+6124 using the Karl G. Jansky Very Large Array radio telescope in New Mexico and NASA’s Swift space telescope.
Study co-author Associate Professor James Miller-Jones, from Curtin University’s node of the International Centre for Radio Astronomy Research (ICRAR) said:
“Neutron stars are stellar corpses.
“They’re formed when a massive star runs out of fuel and undergoes a supernova, with the central parts of the star collapsing under their own gravity.
“This collapse causes the star’s magnetic field to increase in strength to several trillion times that of our own Sun, which then gradually weakens again over hundreds of thousands of years.”
An artist’s impression of the strong magnetic field neutron star in Swift J0243.6+6124 launching a jet. During the bright outburst event in which it was first discovered, the neutron star in Swift J0243.6+6124 was accreting at a very high rate, producing copious X-ray emission from the inner parts of the accretion disk. At the same time, the team detected radio emission with a sensitive radio telescope, the Karl G. Jansky Very Large Array in the USA. By studying how this radio emission changed with the X-rays, we could deduce that it came from fast-moving, narrowly-focused beams of material known as jets, seen here moving away from the neutron star magnetic poles. (Image: ICRAR via University of Amsterdam)
University of Amsterdam Ph.D. student Jakob van den Eijnden, who led the research, said neutron stars and black holes are sometimes found in orbit with a nearby “companion” star, adding:
“Gas from the companion star feeds the neutron star or black hole and produces spectacular displays when some of the material is blasted out in powerful jets travelling at close to the speed of light.”
Visualization of the outburst of the binary system Swift J0243.6+6124 from ICRAR on Vimeo.
Neutron star jets
Astronomers have known about jets for decades, but until now, they had only observed jets coming from neutron stars with much weaker magnetic fields. The prevailing belief was that a sufficiently strong magnetic field prevents material getting close enough to them to form jets. Van den Eijnden said:
“Black holes were considered the undisputed kings of launching powerful jets, even when feeding on just a small amount of material from their companion star.
“The weak jets belonging to neutron stars only become bright enough to see when the star is consuming gas from its companion at a very high rate.
“The magnetic field of the neutron star we studied is about 10 trillion times stronger than that of our own Sun, so for the first time ever, we have observed a jet coming from a neutron star with a very strong magnetic field.
“The discovery reveals a whole new class of jet-producing sources for us to study.”
An artist’s impression of the binary system Swift J0243.6+6124. A binary system with a neutron star in a 27-day orbit and a more massive, rapidly-rotating donor star. The rapid rotation of the donor star throws off a disk of material around the stellar equator. As the neutron star passes through the disk during its orbit, it picks up some of this outflowing gas, which then spirals in toward the neutron star in an accretion disk. (Image: ICRAR via University of Amsterdam)
Astronomers around the world study jets to better understand what causes them and how much power they release into space. Associate Professor Miller-Jones said:
“Jets play a really important role in returning the huge amounts of gravitational energy extracted by neutron stars and black holes back into the surrounding environment.
“Finding jets from a neutron star with a strong magnetic field goes against what we expected, and shows there’s still a lot we don’t yet know about how jets are produced.”
Narrated animation describing the findings and what they mean (English) from ICRAR on Vimeo.
Provided by: International Centre for Radio Astronomy Research (ICRAR) [Note: Materials may be edited for content and length.]
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