'Transformer' Pulsar swaps Radio Waves for Gamma Rays
22 Jul 2014
These artist's renderings show one model of pulsar J1023 before (top) and after (bottom) its radio emission vanished. Normally, the pulsar's wind staves off a gas stream from its companion. When the stream surges, an accretion disk forms and gamma-ray particle jets (magenta) obscure the radio beam. Credit: NASA's Goddard Space Flight Center.
Video: Zoom into AY Sextantis, a binary star system whose pulsar switched from radio emissions to high-energy gamma rays in 2013. This transition likely means the pulsar's spin-up process is nearing its end. Credit: NASA's Goddard Space Flight Center.
In late June 2013, an exceptional binary system containing a rapidly spinning neutron star underwent a dramatic change in behaviour never before observed. Observations with Jodrell Bankís Lovell Telescope showed the pulsar's radio beacon vanished, while at the same time NASA's Fermi Gamma-ray Space Telescope showed the system brightened fivefold in gamma rays.
"It's almost as if someone flipped a switch, morphing the system from a lower-energy state to a higher-energy one," said Professor Ben Stappers, an astrophysicist at the University of Manchester, who led an international effort to understand this striking transformation.
"The change appears to reflect an erratic interaction between the pulsar and its companion, one that allows us an opportunity to explore a rare transitional phase in the life of this binary."
A binary system consists of two stars orbiting around their common centre of mass. This binary, known as AY Sextantis, is located about 4,400 light-years away in the constellation Sextans. It pairs a 1.7-millisecond pulsar named PSR J1023+0038 - J1023 for short - with a star containing about one-fifth the mass of the sun. The two stars complete an orbit in only 4.8 hours, which places them so close together that the emissions from the pulsar will gradually evaporate its companion.
When a massive star collapses and explodes as a supernova, its crushed core may survive as a compact remnant called a neutron star or pulsar, an object squeezing more mass than the Sun contains into a sphere no larger than a city, only about 20 km across. Young isolated neutron stars rotate tens of times each second and generate beams of radio, visible light, X-rays and gamma rays that astronomers observe as pulses whenever the beams sweep past Earth. Pulsars also generate powerful outflows, or "winds," of high-energy particles moving near the speed of light. The power for all this comes from the pulsar's rapidly spinning magnetic field, and over time, as the pulsars slow down, these emissions fade.
More than 30 years ago, astronomers discovered another type of pulsar revolving in 10 milliseconds or less, reaching rotational speeds up to 43,000 rpm. While young pulsars usually appear in isolation, more than half of these millisecond pulsars occur in binary systems, which suggested an explanation for their rapid spin.
"Astronomers have long suspected millisecond pulsars were spun up through the transfer and accumulation of matter from their companion stars, so we often refer to them as recycled pulsars," explained Anne Archibald, a postdoctoral researcher at the Netherlands Institute for Radio Astronomy (ASTRON) in Dwingeloo who discovered J1023 in 2007.
During the initial mass-transfer stage, the system would be classified as a low-mass X-ray binary with a slowly spinning neutron star, one emitting X-ray pulses as hot gas raced toward its surface. A billion years later, when the flow of matter comes to a halt, the system would be identified as a spun-up millisecond pulsar with radio emissions powered by the rapidly rotating magnetic field.
To better understand J1023's spin and orbital evolution, the system was regularly monitored in radio using the University of Manchesterís Lovell Telescope in the United Kingdom and the Westerbork Synthesis Radio Telescope in the Netherlands. These observations revealed that the pulsar's radio signal had turned off and prompted the search for an associated change in its gamma-ray properties.
A few months before this, astronomers found a much more distant system that flipped between radio and X-ray states in a matter of weeks. Located in M28, a globular star cluster about 19,000 light-years away, a pulsar known as PSR J1824-2452I underwent an X-ray outburst in March and April 2013. As the X-ray emission dimmed in early May, the pulsar's radio beam emerged.
While J1023 reached much higher energies and is considerably closer, both binaries are otherwise quite similar. What's happening, astronomers say, are the last sputtering throes of the spin-up process for these pulsars.
In J1023, the stars are close enough that a stream of gas flows from the Sun-like star toward the pulsar. The pulsar's rapid rotation and intense magnetic field are responsible for both the radio beam and its powerful pulsar wind. When the radio beam is detectable, the pulsar wind holds back the companion's gas stream, preventing it from approaching too closely. But now and then the stream surges, pushing its way closer to the pulsar and establishing an accretion disk.
Gas in the disk becomes compressed and heated, reaching temperatures hot enough to emit X-rays. Next, material along the inner edge of the disk quickly loses orbital energy and descends toward the pulsar. When it falls to an altitude of about 80 km, processes involved in creating the radio beam are either shut down or, more likely, obscured.
The inner edge of the disk probably fluctuates considerably at this altitude. Some of it may become accelerated outward at nearly the speed of light, forming dual particle jets firing in opposite directions -- a phenomenon more typically associated with accreting black holes. Shock waves within and along the periphery of these jets are a likely source of the bright gamma-ray emission detected by Fermi.
The findings were published in the July 20 edition of The Astrophysical Journal. The team reports that J1023 is the first example of a transient, compact, low-mass gamma-ray binary ever seen. The researchers anticipate that the system will serve as a unique laboratory for understanding how millisecond pulsars form and for studying the details of how accretion takes place on neutron stars.
"So far, Fermi has increased the number of known gamma-ray pulsars by about 20 times and doubled the number of millisecond pulsars within in our galaxy," said Julie McEnery, the project scientist for the mission at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "Fermi continues to be an amazing engine for pulsar discoveries."
- Download HD video and additional images from NASA Goddard's Scientific Visualization Studio
- Paper: "A State Change In The Missing Link Binary Pulsar System PSR J1023+0038"
- Paper: "A Radio Pulsar/X-ray Binary Link"
- Pulsar Research group at Jodrell Bank
- The Lovell Telescope at Jodrell Bank
- "With A Deadly Embrace, 'Spidery' Pulsars Consume Their Mates" (02.20.2014)
- Interactive: Fermi Pulsar Explorer
- List of rotation- and accretion-powered millisecond pulsars
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