The news in question was that a run-of the-mill pulsar (spinning neutron star) suddenly started violently bursting and hiccuping at X-ray and gamma-ray wavelengths, revealing itself to be a "magnetar" in disguise. The news release was written by former S&T senior editor Bob Naeye, now working at the NASA/Goddard Space Flight Center, and it's such a nice popular exposition of a brain-boggling subject that I'll post the whole thing:
One Weird Star Starts Acting Like Another
[Neutron stars, superdense objects like giant atomic nuclei,] form when the core of a huge star stops producing energy. Gravity collapses the core to form the neutron star. The rest of the star blows up in a stupendously powerful explosion called a supernova.
Neutron stars are made of stuff unllike anything on Earth. These objects pack about one to two Suns worth of material into a ball no larger than New York City. A few cups of neutron star stuff would outweigh Mount Everest.
For years, astronomers have known that some neutron stars emit regular pulses. They essentially go beep-beep-beep-beep-beep, with a perfectly regular spacing between each beep. These neutron stars are known as pulsars, for their pulsing signals. Pulsars spin very rapidly, and it’s [braking action drawing on this rapid spin] that provides the energy for their pulses.
In the 1990s, astronomers discovered a different kind of neutron star. These objects spin slower than pulsars. Because they spin slower, they must be drawing most of their energy from a different kind of source. This source is magnetism. Magnetars are the most magnetic known objects in the entire universe.
Until now, pulsars and magnetars seemed to form two separate classes. A neutron star was either a pulsar or a magnetar, but not both. But using NASA’s Rossi X-ray Timing Explorer (RXTE), astronomers have found a neutron star that seems to share characteristics of both types.
This neutron star is known as PSR J1846-0258. “PSR” is short for “pulsar,” and the numbers stand for its sky location in the constellation Aquila. It lies in a young supernova remnant named Kes 75. For years, PSR J1846 seemed like an ordinary pulsar, beeping three times per second as it spins on its axis.
But a team of Canadian and American astronomers led by Fotis Gavriil of NASA’s Goddard Space Flight Center in Greenbelt, Md., decided to take a closer look. They realized that RXTE observed this pulsar in 2006, but nobody had looked at the observations in detail. When Gavriil and his colleagues studied these observations, they realized that PSR J1846 gave off five huge outbursts of energy. Four of these bursts occurred on May 31, 2006, and the other on July 27, 2006. Each of these flares lasted less than one second, yet during these moments they unleashed the energy of tens of thousands of Suns!
Ordinary pulsars have never been seen to produce such violent bursts of energy. But magnetars generate them frequently. "We are watching one type of neutron star literally change into another right before our very eyes. This is a long-sought missing link between different types of pulsars," says Gavriil.
"Young, fast-spinning pulsars were not thought to have enough magnetic energy to generate such powerful bursts," says team member Marjorie Gonzalez, who is now based at the University of British Columbia in Vancouver, Canada. "Here’s a normal pulsar that’s acting like a magnetar."
Astronomers know that PSR J1846 is very young. It is no more than 884 years old, which is very young compared to most objects in the universe. Maybe magnetars are just a phase of a young neutron star’s life cycle. In other words, maybe a neutron star starts off as a magnetar, but doesn’t start producing outbursts until it's several hundred years old. It acts like a magnetar for perhaps a few thousand years, and then settles down and becomes a pulsar.