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(video animation and interview below) May 20, 1998: When you have eliminated all other possibilities, Sherlock Holmes instructed, whatever remains, however improbable, must be the answer. In the mysterious case of the Soft Gamma Repeaters, or SGRs, the answer appears to be a magnetar, a neutron star with a super-strong magnetic field a thousand trillion times stronger than Earth's. Indeed the magnetic field actually slows the star's rotation and causes starquakes that pump enough energy into the surrounding gases to generate bursts of soft gamma radiation. These led to discovery of the first SGR in 1979. For almost two decades, scientists speculated about the source, and eventually proposed a new class of highly magnetized stars - magnetars. Right: Compton Gamma Ray Observatory, Rossi X-ray Timing Explorer, and the Advanced Satellite for Cosmology and Astrophysics. |
"The importance of this discovery goes beyond just adding a new oddity to the list of star types," said Dr. Chryssa Kouveliotou, the lead scientist on the discovery. "It ties together two rare, very peculiar classes of stars we have been puzzling over, and puts the evolution of neutron stars and even galaxies in a new light." It may also swell the population of our galaxy to include a few hundred million undiscovered magnetars. In the May 21 issue of Nature magazine, Kouveliotou and her colleagues describe how they eliminated the other possibilities to make the "Discovery of an X-ray pulsar with a superstrong magnetic field in the Soft Gamma Repeater called SGR 1806-20." |
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Kouveliotou works for the Universities Space Research Association (USRA) at NASA's Marshall Space Flight Center. Working with her were Dr. Jan van Paradijs of of the University of Amsterdam and the University of Alabama in Huntsville, Dr. Stefan Dieters of the University of Alabama in Huntsville, both working at NASA's Marshall Space Flight Center (MSFC) in Huntsville Ala., and Dr. Tod Strohmayer of NASA's Goddard Space Flight Center in Greenbelt, Md. Looking for a suspect Their find strongly supports the magnetar theory offered in 1992 by astrophysicists Dr. Robert Duncan of the University of Texas at Austin and Dr. Christopher Thompson of the University of North Carolina at Chapel Hill. It's a dynamic model that has the neutron star going through a violent afterlife lasting about 10,000 years. Many colleagues discounted the concept, saying that internal pressures and other factors would keep a star from generating such an intense field. |
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Credit NASA/Marshall Space Flight Center Requires Realvideo player (version 5). Click to download the RealVideo Player (from RealNetworks, Inc. ![]() |
![]() Above: SGR 1806-20 has been the most energetic of the Soft Gamma Repeaters, but not the only one. The image at left links to a 1404x946-pixel, 160KB plot showing the time histories of the three confirmed SGRs. Note that the scales for the two bottom plots are only 1/10th as high as for SGR 1806-20. (credit: Kouveliotou, NASA & USRA) |
Theories abounded, but no one could be certain of the cause. So, it remained what Holmes would call "quite a three-pipe problem" until it became a three-satellite problem 10 years later. In November 1996, the Burst and Transient Source Experiment aboard the Compton Gamma Ray Observatory detected SGR 1806-20 flaring up again. Kouveliotou used time she was allotted on Rossi X-ray Timing Explorer to take a closer look at the X-ray activities that followed. During Nov. 5-18, 1996, RXTE captured several hours worth of data as bursts came in a "bunching" mode that had not been seen before. Following her observations, RXTE kept watching SGR 1806-20 to provide data for Strohmayer who was allotted time to observe during SGR 1806-20's quiescent phase. The result was a complementary data set that led to collaboration. "Combining our data gave us both the capability to make a more sensitive search as well as provide a way to verify each others analysis of the data," said Strohmayer. Reading the evidenceAs the name implies, RXTE carries instruments that read data quickly. Where most telescopes really take time exposures, RXTE Proportional Counter Array acts like a fast electronic counter which, combined with its size, was highly effective in searching for a pattern in the X-rays. "I found a candidate periodic signal at 7.5 seconds in Chryssa's data, but we needed to have confirmation that the signal was also in Tod's dataset before we would be convinced it was real," remarked Dieters. The study was complicated by the need to carefully remove the data segments which had SGR bursts in them. "When you're looking for such a weak pulsar signal, the bursts could totally mask the modulations."
"When you know what period you are looking for it gives you a great advantage in sensitivity," remarked Strohmayer. "Finding the pulsed signal in the RXTE data allowed us to go back and also find it in the ASCA data, this removed the last shred of doubt that the pulsed signal could possibly be from another, previously unknown object in the RXTE field of view." Between the ASCA and RXTE observations, SGR 1806-20 had slowed by 8/1,000th of a second. The difference would be miniscule except that it happened in less than four years to an object with more mass than our sun. To test her finding, Kouveliotou asked Jeff Kommers of the Massachusetts Institute of Technology, another colleague, to check the data. Using a different approach, he came up with 7.5-seconds. "That was the clincher," Kouveliotou said. "Two good data sets and two different methods of analysis gave the same answer." Having established that SGR 1806-20 is associated with a pulsar and is slowing, rapidly, the team asked what might fit that profile. In science, proving what something is often involves proving what it is not. Scientists suspected that SGRs are magnetars, but first they had to eliminate objects other than pulsars as the sources, and then eliminate possibilities other than magnetars as the answer. The first possibility was simple accretion where material from another star is scooped up by the pulsar, or the magnetar. Radio telescope observations by team member Dale Frail at the National Radio Astronomy Observatory helped rule out the accretion model. He showed that SGR 1806-20 coincides with a supernova remnant, SNR G10.0-0.3, whose radio broadcasts suggest a compact shape. It is also may be orbiting a nearby massive blue star every 10 years. But 1806's own stellar wind is too powerful to let material fall inward, so it can't be an accreting pulsar.
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"Third, their pulse periods were close together," said van Paradijs. "All of them were like 6 to 10 seconds, which is very different from what you find with normal X-ray pulsars, which have pulse periods as short as less than a tenth of a second and as long as half an hour." Since they slow down rapidly, then only a handful would be active for us to observe. "So that even though there may be many of them, most of them are inactive, dead, so to say, lying in the graveyard," van Paradijs said. If the 10 or so SGRs and AXPs are magnetars, each less than 10,000 years old, then they probably form about once every thousand years. "I think that conservatively 1 million magnetars have formed in our galaxy, and perhaps as many as 30 to 100 million," Duncan added. Many of the supernova remnants that lack pulsars actually have them in the form of invisible, dead pulsars that exploded as supernovas, sputtered as SGRs concealing magnetars, then faded through the AXP stage to become invisible. Some may be made visible with more sensitive instruments like NASA/Marshall's Advanced X-ray Astrophysics Facility slated for launch in December 1997. "Our plans are to go back to that source with RXTE, and hopefully with AXAF, and make more sensitive observations," Kouveliotou. "This is just starting. I'm looking forward to a hot debate on the subject." |
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Click your network speed for most appropriate movie: Credit Dr. Robert Mallozzi /UAH and NASA/Marshall Space Flight Center Requires Realvideo player (version 5). Click to download the RealVideo Player (from RealNetworks, Inc. ![]() Animated Gif movies available (shows short segment of burst animation) |
Authors on the Nature paper are Dr. Chryssa Kouveliotou
of the Universities Space Research Association, Dr. Jan van Paradijs
and Dr. Stefan Dieters of the University of Alabama in Huntsville,
Dr. Tod Strohmayer of NASA's Goddard Space Flight Center, Dr.
Gerald Fishman and Dr. Charles Meegan, both of Marshall Space
Flight Center, Dr. Kevin Hurley of the University of California
at Berkeley, and Dr. Jeff Kommers of the Massachusetts Institute
of Technology, Dr. Ian Smith of Rice University, Dr. Dale Frail
of the National Radio Astronomy Observatory, and Dr. Toshio Murakami
of Japan's Institute of Space and Astronautical Sciences.
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