Observations from the European Southern Observatory’s (ESO) La Silla and Paranal Observatories in Chile have for the first time demonstrated a link between a long-lasting burst of gamma rays and an unusually bright supernova explosion. The results show that the supernova was not driven by radioactive decay, as expected, but was instead powered by the decaying super-strong magnetic fields around an exotic object called a magnetar.
Gamma-ray bursts (GRBs) are one of the outcomes associated with the biggest explosions to have taken place since the Big Bang. They are detected by orbiting telescopes that are sensitive to this type of high-energy radiation, which cannot penetrate Earth’s atmosphere, and then observed at longer wavelengths by other telescopes both in space and on the ground.
GRBs usually only last a few seconds, but in very rare cases the gamma rays continue for hours. One such ultra-long-duration GRB was picked up by the Swift satellite on December 9, 2011, and named GRB 111209A. It was both one of the longest and brightest GRBs ever observed.
As the afterglow from this burst faded, it was studied using both the GROND instrument on the MPG/ESO 2.2-meter telescope at La Silla and also with the X-shooter instrument on the Very Large Telescope (VLT) at Paranal. The clear signature of a supernova, later named SN 2011kl, was found. This is the first time that a supernova has been found to be associated with an ultra-long GRB.
“Since a long-duration gamma-ray burst is produced only once every 10,000–100,000 supernovae, the star that exploded must be somehow special,” said Jochen Greiner from the Max Planck Institute for Extraterrestrial Physics in Garching, Germany. “Astronomers had assumed that these GRBs came from very massive stars — about 50 times the mass of the Sun — and that they signaled the formation of a black hole. But now our new observations of the supernova SN 2011kl, found after the GRB 111209A, are changing this paradigm for ultra-long-duration GRBs.”
In the favored scenario of a massive star collapse — sometimes known as a collapsar — the weeklong burst of optical/infrared emission from the supernova is expected to come from the decay of radioactive nickel-56 formed in the explosion. But in the case of GRB 111209A, the combined GROND and VLT observations showed unambiguously for the first time that this could not be the case. Other suggestions were also ruled out.
The only explanation that fitted the observations of the supernova following GRB 111209A was that it was being powered by a magnetar — a tiny neutron star spinning hundreds of times per second and possessing a magnetic field much stronger than normal neutron stars, which are also known as radio pulsars. Magnetars are thought to be the most strongly magnetized objects in the known universe. This is the first time that such an unambiguous connection between a supernova and a magnetar has been possible.
“The new results provide good evidence for an unexpected relation between GRBs, very bright supernovae, and magnetars,” said Paolo Mazzali. “Some of these connections were already suspected on theoretical grounds for some years, but linking everything together is an exciting new development.”
“The case of SN 2011kl/GRB 111209A forces us to consider an alternative to the collapsar scenario. This finding brings us much closer to a new and clearer picture of the workings of GRBs,” said Greiner.